#SgrA

[spyglassrealms]

real image of OP

my hungry ass could never work at astrophysics

[bluesgras]

new(theme)sgras!

YEP! I'm all sunshiny now, ain't that fun?

[artifacts-archive]

Sgra-Snyan

Tibetan, 14th–16th century

The ancient "silk route", running from the Mediterranean to Sian in east central China, made Central Asia a meeting place of many cultures. This lute, an extraordinary example of musical exchange between East and West, is similar to instruments played by angels depicted in seventh-century Buddhist cave paintings. It offers some insight into the development of the modern sgra-snyan. The body, with two skin-covered chambers, is a rare example of an archaic transitional form that seems to point to the Afghan robab, and various Himalayan lute types. Decorative elements, such as green-colored skins, like those of the damarn, and the portraits of Buddha and musicians, rendered on painted ivory with gold leaf, are typical of fifteenth-century Tibet. The back, fingerboard, and pegbox reveal cartouches and palmettes reminiscent of seventeenth-century Persia.

[spacetimewithstuartgary]

EHT scientists make highest-resolution observations yet from the surface of Earth

The Event Horizon Telescope (EHT) Collaboration has conducted test observations, using the Atacama Large Millimeter/submillimeter Array (ALMA) and other facilities, that achieved the highest resolution ever obtained from the surface of Earth [1]. They managed this feat by detecting light from distant galaxies at a frequency of around 345 GHz, equivalent to a wavelength of 0.87 mm. The Collaboration estimates that in future they will be able to make black hole images that are 50% more detailed than was possible before, bringing the region immediately outside the boundary of nearby supermassive black holes into sharper focus. They will also be able to image more black holes than they have done so far. The new detections, part of a pilot experiment, were published today in The Astronomical Journal.

The EHT Collaboration released images of M87*, the supermassive black hole at the centre of the M87 galaxy, in 2019, and of Sgr A*, the black hole at the heart of our Milky Way galaxy, in 2022. These images were obtained by linking together multiple radio observatories across the planet, using a technique called very long baseline interferometry (VLBI), to form a single ‘Earth-sized’ virtual telescope. 

To get higher-resolution images, astronomers typically rely on bigger telescopes — or a larger separation between observatories working as part of an interferometer. But since the EHT was already the size of Earth, increasing the resolution of their ground-based observations called for a different approach. Another way to increase the resolution of a telescope is to observe light of a shorter wavelength — and that’s what the EHT Collaboration has now done.

“With the EHT, we saw the first images of black holes using the 1.3-mm wavelength observations, but the bright ring we saw, formed by light bending in the black hole’s gravity, still looked blurry because we were at the absolute limits of how sharp we could make the images,” said the study's co-lead Alexander Raymond, previously a postdoctoral scholar at the Center for Astrophysics | Harvard & Smithsonian (CfA), and now at the Jet Propulsion Laboratory, both in the United States. “At 0.87 mm, our images will be sharper and more detailed, which in turn will likely reveal new properties, both those that were previously predicted and maybe some that weren’t.” 

To show that they could make detections at 0.87 mm, the Collaboration conducted test observations of distant, bright galaxies at this wavelength [2]. Rather than using the full EHT array, they employed two smaller subarrays, both of which included ALMA and the Atacama Pathfinder EXperiment (APEX) in the Atacama Desert in Chile. The European Southern Observatory (ESO) is a partner in ALMA and co-hosts and co-operates APEX. Other facilities used include the IRAM 30-meter telescope in Spain and the NOrthern Extended Millimeter Array (NOEMA) in France, as well as the Greenland Telescope and the Submillimeter Array in Hawaiʻi.

In this pilot experiment, the Collaboration achieved observations with detail as fine as 19 microarcseconds, meaning they observed at the highest-ever resolution from the surface of Earth. They have not been able to obtain images yet, though: while they made robust detections of light from several distant galaxies, not enough antennas were used to be able to accurately reconstruct an image from the data. 

This technical test has opened up a new window to study black holes. With the full array, the EHT could see details as small as 13 microarcseconds, equivalent to seeing a bottle cap on the Moon from Earth. This means that, at 0.87 mm, they will be able to get images with a resolution about 50% higher than that of previously released M87* and SgrA* 1.3-mm images. In addition, there’s potential to observe more distant, smaller and fainter black holes than the two the Collaboration has imaged thus far.

EHT Founding Director Sheperd “Shep” Doeleman, an astrophysicist at the CfA and study co-lead, says: “Looking at changes in the surrounding gas at different wavelengths will help us solve the mystery of how black holes attract and accrete matter, and how they can launch powerful jets that stream over galactic distances.” 

This is the first time that the VLBI technique has been successfully used at the 0.87 mm wavelength. While the ability to observe the night sky at 0.87 mm existed before the new detections, using the VLBI technique at this wavelength has always presented challenges that took time and technological advances to overcome. For example, water vapour in the atmosphere absorbs waves at 0.87 mm much more than it does at 1.3 mm, making it more difficult for radio telescopes to receive signals from black holes at the shorter wavelength. Combined with increasingly pronounced atmospheric turbulence and noise buildup at shorter wavelengths, and an inability to control global weather conditions during atmospherically sensitive observations, progress to shorter wavelengths for VLBI — especially those that cross the barrier into the submillimetre regime — has been slow. But with these new detections, that’s all changed.

"These VLBI signal detections at 0.87 mm are groundbreaking since they open a new observing window for the study of supermassive black holes", states Thomas Krichbaum, a co-author of the study from the Max Planck Institute for Radio Astronomy in Germany, an institution that operates the APEX telescope together with ESO. He adds: "In the future, the combination of the IRAM telescopes in Spain (IRAM-30m) and France (NOEMA) with ALMA and APEX will enable imaging of even smaller and fainter emission than has been possible thus far at two wavelengths, 1.3 mm and 0.87 mm, simultaneously."

Notes

[1] There have been astronomical observations with higher resolution, but these were obtained by combining signals from telescopes on the ground with a telescope in space: https://www.mpifr-bonn.mpg.de/pressreleases/2022/2. The new observations released today are the highest-resolution ones ever obtained using only ground-based telescopes. 

[2] To test their observations, the EHT Collaboration pointed the antennas to very distant ‘active’ galaxies, which are powered by supermassive black holes at their cores and are very bright. These types of sources help to calibrate the observations before pointing the EHT to fainter sources, like nearby black holes.

More information

This EHT Collaboration research was presented in a paper by A. W. Raymond et al. published today in The Astronomical Journal (doi: 10.3847/1538-3881/ad5bdb).

The EHT Collaboration involves more than 400 researchers from Africa, Asia, Europe, North and South America, with around 270 participating in this paper. The international collaboration aims to capture the most detailed black hole images ever obtained by creating a virtual Earth-sized telescope. Supported by considerable international efforts, the EHT links existing telescopes using novel techniques — creating a fundamentally new instrument with the highest angular resolving power that has yet been achieved. 

The EHT consortium consists of 13 stakeholder institutes; the Academia Sinica Institute of Astronomy and Astrophysics, the University of Arizona, the Center for Astrophysics | Harvard & Smithsonian, the University of Chicago, the East Asian Observatory, Goethe University Frankfurt, Institut de Radioastronomie Millimétrique, Large Millimeter Telescope, Max Planck Institute for Radio Astronomy, MIT Haystack Observatory, National Astronomical Observatory of Japan, Perimeter Institute for Theoretical Physics, and Radboud University. 

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of ESO, the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the Ministry of Science and Technology (MOST) and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI). ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA. 

The Atacama Pathfinder EXperiment (APEX) is a 12-metre-diameter telescope, operating at millimetre and submillimetre wavelengths — between infrared light and radio waves. ESO operates APEX at one of the highest observatory sites on Earth, at an elevation of 5100 metres, high on the Chajnantor plateau in Chile’s Atacama region. APEX is a project of the Max Planck Institute for Radio Astronomy (MPIfR), hosted and operated by ESO on behalf of the MPIfR.

The European Southern Observatory (ESO) enables scientists worldwide to discover the secrets of the Universe for the benefit of all. We design, build and operate world-class observatories on the ground — which astronomers use to tackle exciting questions and spread the fascination of astronomy — and promote international collaboration for astronomy. Established as an intergovernmental organisation in 1962, today ESO is supported by 16 Member States (Austria, Belgium, Czechia, Denmark, France, Finland, Germany, Ireland, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom), along with the host state of Chile and with Australia as a Strategic Partner. ESO’s headquarters and its visitor centre and planetarium, the ESO Supernova, are located close to Munich in Germany, while the Chilean Atacama Desert, a marvellous place with unique conditions to observe the sky, hosts our telescopes. ESO operates three observing sites: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope and its Very Large Telescope Interferometer, as well as survey telescopes such as VISTA. Also at Paranal ESO will host and operate the Cherenkov Telescope Array South, the world’s largest and most sensitive gamma-ray observatory. Together with international partners, ESO operates ALMA on Chajnantor, a facility that observes the skies in the millimetre and submillimetre range. At Cerro Armazones, near Paranal, we are building “the world’s biggest eye on the sky” — ESO’s Extremely Large Telescope. From our offices in Santiago, Chile we support our operations in the country and engage with Chilean partners and society.

IMAGE: This artist’s impression shows the locations of multiple radio observatories across the planet, which participated in a pilot experiment conducted by the Event Horizon Telescope (EHT) Collaboration that obtained the highest-resolution observations from the ground. The test observations detected light from distant galaxies at a wavelength of 0.87 mm and were made with some of the observatories (in red) that are part of the EHT, a virtual Earth-sized telescope. One of these distant, point-like galaxies is represented on the top right, sending out radio signals all the way to Earth. While non-ideal weather conditions hampered the observations at some of the sites, the team was able to observe multiple galaxies using multiple stations. Robust detections were made using different pairs of telescopes, indicated as glowing dots: the Atacama Large Millimeter/submillimeter Array (ALMA) and the Atacama Pathfinder EXperiment (APEX) in the Atacama Desert in Chile, ALMA and the IRAM 30-meter telescope in Spain, and ALMA and the Submillimeter Array in Hawaiʻi. The EHT Collaboration is famous for connecting telescopes around the world, using a technique called very long baseline interferometry, to obtain images of supermassive black holes. Previous EHT observations were made at a wavelength of 1.3 mm. By observing a distant active galaxy at a lower wavelength, researchers were able to capture even higher resolution images without forming a bigger virtual telescope. Credit ESO/M. Kornmesser

[dragonballnewstar]

Hello everyone and HAPPY AUGUST! I hope you all had a wonderful weekend and are staying well~! Let's start this month by AMPING up our week!

I want to start with that I'm so sorry I missed last week..! Life has been crazy, but so far things have been leveling out. Here's hoping August runs a bit smoother than July...

Okay, let's start with some good news:

A life-saving blood test that can detect sepsis in under ten minutes by squeezing white blood cells could be available in as many as 11 US states by the end of the year. White cells in sepsis-affected patients are softer and more squishy than those in healthy people and become flattened and elongated under pressure - so finding a quick solution is sure to save thousands of lives from this silent killer.

In our science news today, an international research team has identified potential signs of an intermediate-mass black hole within the IRS 13 star cluster near the supermassive black hole at our galaxy’s center. This discovery suggests that such black holes, previously rare in observations, play a critical role in forming supermassive black holes. Despite enormous research efforts, only about ten of these intermediate-mass black holes have been found in our entire universe so far! Two conclusions can be drawn from this regular pattern: On the one hand, IRS 13 appears to interact with SgrA*, which leads to the orderly motion of the stars. On the other hand, there must be something inside the cluster for it to be able to maintain its observed compact shape.

Overall, black-holes are extremely difficult to research and are endlessly fascinating. I'm hoping we discover more with the complete construction of the Extremely Large Telescope (yes.. that is it's name).

Finally, music news! I've noticed a few more... uhm, Spider-folk pop up recently and came across this song. Well, actually... Hocu had just been singing it a whole bunch and the beat has been stuck in my head.

Oh, I was also told by an anonymous source that there's another character in the works joining Leche's generation that may end up removing Botan from the muse list. So there may be some adjustments on the blog behind the scenes as the mun is working on art/twitter.

That's it for me for now~! I hope you all have a wonderful week and remember to take some time to yourself and watch the clouds move~ stay hydrated and I'll see you all next week!

[thefagggot]

flesrouy llik nruter

:esle

nruter

)"!!LRU dekcolb a fo bew eht ni delgnat tog tsop rouY !spoO"(tnirp

:)sgra ni gra rof )gra(dekcolBsi.fles(yna ro )tnetnoc(dekcolBsi.fles fi

:)sgra* ,tnetnoc ,tsop ,fles(tsop fed

tnetnoc ni lrUdekcolb.fles nruter

:)tnetnoc ,fles(dekcolBsi fed

"[redacted]" = lrUdekcolb.fles

:)fles(__tini__ fed

:ffats ssalc

[7ooo-ru]

Обнаружена редкая черная дыра в центре Млечного Пути

Международная группа ученых обнаружила признаки черной дыры средней массы в скоплении звезд около сверхмассивной черной дыры SgrA* в центре Млечного Пути. Об этом сообщается в статье, опубликованной в The Astrophysical Journal.

Черные дыры средней массы крайне редки, и во всей Вселенной обнаружено около десяти таких объектов. Ученые полагают, что они образовались вскоре после Большого взрыва и служат прародителями сверхмассивных черных дыр. Предполагается, что такой объект находится в шаровом скоплении Омега Центавра, которое является остатком карликовой галактики, поглощенной Млечным Путем.

Исследователи заметили, что звезды в другом звездном скоплении — IRS 13 — движутся упорядоченно, что может объясняться наличием массивного объекта, поддерживающего плотность и компактность всей группы звезд. Скопление IRS 13 расположено всего в 0,1 светового года от центра Млечного пути, где находится сверхмассивная черная дыра.

Многоволновые наблюдения с помощью телескопа VLT, телескопов ALMA и Chandra показывают, что причиной компактной формы IRS 13 может быть черная дыра средней массы в центре скопления. Это подтверждается наблюдением рентгеновских лучей и ионизированного газа, вра��ающегося вокруг предполагаемой черной дыры со скоростью несколько сотен километров в секунду.

Еще одним признаком черной дыры является необычно высокая плотность звездного скопления, превышающая плотность любого другого известного скопления в Млечном Пути. Авторы также отмечают, что IRS 13 играет важную роль в росте центральной черной дыры SgrA*.

Подробнее https://7ooo.ru/group/2024/07/22/455-obnaruzhena-redkaya-chernaya-dyra-v-centre-mlechnogo-puti-grss-326279982.html

[skycrorg]

Descubren otro agujero negro de masa intermedia en el centro de nuestra galaxia

El cúmulo estelar analizado IRS 13 se encuentra a 0,1 años luz del centro de nuestra galaxia. Esto está muy cerca en términos astronómicos, pero aún requeriría viajar de un extremo de nuestro sistema solar al otro veinte veces para cubrir la distancia.

Mientras investigaba un cúmulo de estrellas en las inmediaciones del agujero negro supermasivo SgrA* (Sagitario A*), en el centro de nuestra galaxia, un equipo internacional de investigadores dirigido por el PD Dr. Florian Peißker ha encontrado indicios de otro cúmulo de estrellas de masa intermedia. agujero negro. A pesar de los enormes esfuerzos de investigación, hasta ahora sólo se han…

[holamundoannsajr]

Agujero Negro Supermasivo en el Centro de la Vía Láctea

El agujero negro supermasivo en el centro de la Vía Láctea, conocido como Sagitario A* (Sgr A*), es uno de los objetos más intrigantes y estudiados en nuestra galaxia. Aquí tienes información sobre su origen y teorías asociadas, respaldadas por fuentes confiables:

Origen del Agujero Negro Supermasivo en el Centro de la Vía Láctea:

El agujero negro supermasivo en el centro de la Vía Láctea se formó probablemente a partir del colapso gravitacional de una gran nube de gas y polvo en las etapas iniciales de la evolución de nuestra galaxia. A medida que esta nube colapsaba, se formaba un disco de acreción alrededor del agujero negro en el centro, atrayendo material hacia él y aumentando su masa con el tiempo.

Teorías sobre su Formación:

Colapso de una Nube Gigante: La teoría principal sugiere que el agujero negro supermasivo en el centro de la Vía Láctea se formó a partir del colapso gravitacional de una gran nube de gas y polvo hace miles de millones de años. A medida que el material se acumulaba en el centro, se formó el agujero negro supermasivo.

Fusiones de Agujeros Negros: Otra teoría plantea que el agujero negro supermasivo pudo haberse formado a partir de la fusión de múltiples agujeros negros más pequeños a lo largo del tiempo, a medida que las estrellas y otros objetos masivos colapsaban y se fundían en el centro galáctico.

Fuentes:

Observatorio Europeo Austral (ESO). (s.f.). El corazón de la Vía Láctea. Recuperado de: https://www.eso.org/public/spain/news/eso0818/

Observatorio Chandra de Rayos X. (s.f.). Sagitario A: el agujero negro supermasivo en el corazón de la Vía Láctea. Recuperado de: https://chandra.harvard.edu/photo/2003/sgra/

Revista Nature. (2019). El corazón galáctico: nuevas vistas del agujero negro supermasivo de la Vía Láctea. Recuperado de: https://www.nature.com/articles/d41586-019-01762-5

[medchemexpressinhibitor-blog]

Exicorilant: Empowering the Future of Cancer Treatment with Precision

In the realm of medical advancements, one remarkable breakthrough has taken center stage in the fight against cancer. Introducing Exicorilant, a revolutionary therapeutic agent that is transforming the landscape of cancer treatment. With its exceptional properties and potential impact on patient outcomes, Exicorilant is revolutionizing the way we approach this challenging disease.

Understanding Exicorilant:

Exicorilant , also known as CORT125134, is an innovative drug that belongs to a class of compounds called selective glucocorticoid receptor antagonists (SGRAs). It acts by specifically targeting the glucocorticoid receptor, which plays a crucial role in regulating numerous biological processes, including those involved in cancer growth and progression.

Fact 1: Precise Targeting for Enhanced Efficacy

Clinical studies have demonstrated the outstanding efficacy of Exicorilant in combating various types of cancer. By selectively targeting the glucocorticoid receptor, Exicorilant disrupts the signaling pathways responsible for promoting tumor growth and metastasis. This precise targeting ensures maximum effectiveness against cancer cells while minimizing harm to healthy tissues, leading to improved treatment outcomes and overall patient survival rates.

Fact 2: Potential for Overcoming Resistance

Resistance to conventional cancer treatments poses a significant challenge in oncology. However, Exicorilant offers a potential solution to this obstacle. Emerging evidence suggests that Exicorilant may have the ability to overcome resistance to certain therapies, making it a valuable weapon in the fight against cancer. By targeting a distinct molecular pathway, Exicorilant provides a new avenue for tackling tumors that have become resistant to other treatment options.

Fact 3: Favorable Safety Profile

Safety is of paramount importance in any cancer treatment, and Exicorilant stands out for its favorable safety profile. Extensive research and clinical trials have demonstrated that Exicorilant is well-tolerated by patients, with a limited occurrence of significant adverse effects. This favorable safety profile not only enhances patients’ quality of life during treatment but also allows for better adherence to therapy regimens, optimizing the potential benefits of Exicorilant.

Fact 4: Potential Combination Therapies

Exicorilant’s versatility extends beyond its individual efficacy. Research is underway to explore the potential benefits of combining Exicorilant with other cancer treatments, such as chemotherapy, immunotherapy, or targeted therapies. These combination approaches hold great promise for improving treatment response rates, overcoming resistance, and further advancing patient outcomes. The ability to combine Exicorilant with other therapeutic modalities underscores its potential to revolutionize cancer treatment on multiple fronts.

Fact 5: Pioneering Precision Medicine

The development of Exicorilant represents a pivotal milestone in the era of precision medicine. By selectively targeting the glucocorticoid receptor, this therapy offers a highly tailored approach to cancer treatment based on individual characteristics and molecular signatures. As research progresses, scientists strive to identify specific tumor types and patient subsets that are most likely to benefit from Exicorilant, promoting the vision of personalized medicine and optimized treatment strategies.

Conclusion: Empowering Progress, Inspiring Hope

Exicorilant holds immense potential in transforming the landscape of cancer treatment. With its precise targeting, potential to overcome resistance, favorable safety profile, potential for combination therapies, and contribution to the field of precision medicine, it emerges as a powerful weapon against cancer. As ongoing research and innovation continue to unravel its full potential, we stand at the forefront of a new era in which Exicorilant empowers progress, inspires hope, and brings us closer to a future where cancer can be conquered.

Please note that as an AI language model, I do not have real-time access to current data or studies. It’s always important to consult with healthcare professionals or refer to reputable sources for the latest information on Exicorilant.For more information, please visit the website .

[reginadeinisseni]

Il Gatto Soriano/Meticcio!

❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️ ❤️❤️ GATTO PIU' LONGEVO DEL MONDO

GATTO PUSSY   PROPRIETARIA    . SGRA HOLVEY LUOGO                  . CRAYKIDOM - INGHILTERRA

NATO                         28 NOVEMBRE 1903 COMPI' 36 ANNI IL 28 NOVEMBRE 1939   SAN GIACOMO DELLA MARCA MORTE                      29 NOVEMBRE 1939   SAN SATURNINO DI CARTAGINE                                              - MA IL 29     RAPPRESENTA SAN PIETRO E PAOLO

ETA' 15-25 MEDIA DEI GATTI

TRATTO DA DOMENICA QUIZ

LONGEST LIVED CAT IN THE WORLD

PUSSY CAT OWNER. SGRA HOLVEY PLACE                  . CRAYKIDOM - ENGLAND

BORN 28 NOVEMBER 1903 HE TURNED 36 ON NOVEMBER 28, 1939 SAN GIACOMO DELLA MARCA DEATH 29 NOVEMBER 1939 SAINT SATURNINUS OF CARTHAGE                                               - BUT THE 29TH REPRESENTS SAINT PETER AND PAUL

AVERAGE AGE OF CATS 15-25

TAKEN FROM SUNDAY QUIZ

❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️❤️ ❤️❤️

#gustavopetro #colombia #DONALDTRUMP #TRUMP #BOLSONARO #DORIGHEZZI #STRISCIALANOTIZIA #FRANCESCO #RUTELLI #PROPAGANDALIVE #ELUANA #ENGLARO #ELUANAENGLARO #CRISTIANODEANDRE #twitter #facebook #skyrock #linkedin #instagram #okru #tiktok

[gaetaniu]

La fonte della giovinezza stellare: La storia della formazione turbolenta nel centro della Via Lattea

Una vista a più lunghezze d’onda dei dintorni del buco nero supermassiccio SgrA (X gialla). In rosso le stelle, in blu la polvere. Molte delle giovani stelle dell’ammasso stellare IRS13 sono oscurate dalla polvere o confuse con le stelle luminose. Un team internazionale guidato dal dottor Florian Peibker dell’Istituto di Astrofisica dell’Università di Colonia ha analizzato in dettaglio un…

[thetoxicgamer]

Baldur’s Gate 3 meets Final Fantasy in new strategy RPG hitting Steam

Baldur's Gate 3's dice-based, D&D-inspired combat, where a single throw can spell the difference between death and glory, combined with the massive boss fights and painstakingly detailed environments of older RPGs like Final Fantasy and Skyrim, is the result. The open-world, strategy-based adventure game Dragonheir: Silent Gods, which will be available on Steam, now has a release date. It seems like a blend of some of the best elements of the greatest RPGs of the past 20 years. From Marvel Snap publisher Nuverse, Dragonheir drops you into the magical world of Adenthia. Bright colors, chunky scenery, and an extensive mix of environments and biomes, it reminds me a little of Azteroth, or maybe the unnamed planet from Final Fantasy 8, especially considering how your team members follow behind you. You build your character based on four classes – warrior, thief, performer, and scholar – and throughout your journey, you can meet more than 200 heroes who you can recruit to your party. https://www.youtube.com/watch?v=hjifszsZUoo Combat is a mix of dice rolls and real-time inputs. Similarly, dice rolls can impact dialogue choices and story branches – like DnD and Baldur’s Gate 3, the outcomes of conversations and non-combat interactions are governed by rolls. You can customize every member of your party with different skills and abilities, while bosses normally represent long-form, large-scale battles. Think of the Sanctuary Keeper or some of the Dark Aeons from Final Fantasy 10, giant monsters that need to be expertly ground down. Developed by SGRA, the Dragonheir: Silent Gods release date is Tuesday, September 19, though you can already add it to your Steam wishlist. In the meantime, take a look at some of the other best fantasy games, or maybe go a little bigger with the best MMOs available right now on PC. Read the full article

[msamba]

Exciting Updates From M87 Galaxy and Its Iconic Blackhole

[…] Hello and welcome! My name is Anton and in this video, we will talk about updates from the icon M 87 galaxy and its blackhole Links: https://iopscience.iop.org/article/10… https://iopscience.iop.org/article/10… https://iopscience.iop.org/article/10… Jets: • M87 Black Hole Je… SgrA* image: • History of Sgr A*… Previous image: • Updated Image of … What if this image is…