#Active Galaxy NGC 1275
Explore tagged Tumblr posts
Photo
Active Galaxy NGC 1275 #NASA https://ift.tt/rPqxJZk
0 notes
Photo
Active Galaxy NGC 1275
Credits: NASA, ESA, Hubble Heritage, STScI, AURA, A. Fabian, IoA, Cambridge U., CXC, NRAO,VLA
78 notes
·
View notes
Photo
Active Galaxy NGC 1275 via NASA https://ift.tt/YkgBtPy
107 notes
·
View notes
Photo
2023 January 26
Active Galaxy NGC 1275 Image Credit: NASA, ESA, Hubble Heritage, A. Fabian (University of Cambridge, UK)
Explanation: Active galaxy NGC 1275 is the central, dominant member of the large and relatively nearby Perseus Cluster of Galaxies. Wild-looking at visible wavelengths, the active galaxy is also a prodigious source of x-rays and radio emission. NGC 1275 accretes matter as entire galaxies fall into it, ultimately feeding a supermassive black hole at the galaxy's core. This color composite image made from Hubble Space Telescope data recorded during 2006. It highlights the resulting galactic debris and filaments of glowing gas, some up to 20,000 light-years long. The filaments persist in NGC 1275, even though the turmoil of galactic collisions should destroy them. What keeps the filaments together? Observations indicate that the structures, pushed out from the galaxy's center by the black hole's activity, are held together by magnetic fields. Also known as Perseus A, NGC 1275 spans over 100,000 light years and lies about 230 million light years away.
∞ Source: apod.nasa.gov/apod/ap230126.html
80 notes
·
View notes
Text
Active Galaxy NGC 1275
Active galaxy NGC 1275 is the central, dominant member of the large and relatively nearby Perseus Cluster of Galaxies. Wild-looking at visible wavelengths, the active galaxy is also a prodigious source of x-rays and radio emissions. NGC 1275 accretes matter as entire galaxies fall into it, ultimately feeding a supermassive black hole at the galaxy's core. This color composite image is made from Hubble Space Telescope data recorded during 2006. It highlights the resulting galactic debris and filaments of glowing gas, some up to 20,000 light-years long. The filaments persist in NGC 1275, even though the turmoil of galactic collisions should destroy them. What keeps the filaments together? Observations indicate that the structures, pushed out from the galaxy's center by the black hole's activity, are held together by magnetic fields. Also known as Perseus A, NGC 1275 spans over 100,000 light years and lies about 230 million light years away.
Image Copyright: Image Credit: NASA, ESA, Hubble Heritage, A. Fabian (University of Cambridge, UK)
15 notes
·
View notes
Photo
Active Galaxy NGC 1275 Active galaxy NGC 1275 is the central, dominant member of the large and relatively nearby Perseus Cluster of Galaxies. Wild-looking at visible wavelengths, the active galaxy is also a prodigious source of x-rays and radio emission. NGC 1275 accretes matter as entire galaxies fall into it, ultimately feeding a supermassive black hole at the galaxy's core. This color composite image made from Hubble Space Telescope data recorded during 2006. It highlights the resulting galactic debris and filaments of glowing gas, some up to 20,000 light-years long. The filaments persist in NGC 1275, even though the turmoil of galactic collisions should destroy them. What keeps the filaments together? Observations indicate that the structures, pushed out from the galaxy's center by the black hole's activity, are held together by magnetic fields. Also known as Perseus A, NGC 1275 spans over 100,000 light years and lies about 230 million light years away.
3 notes
·
View notes
Photo
Active Galaxy NGC 1275 via NASA https://ift.tt/tx5jnlH
Active galaxy NGC 1275 is the central, dominant member of the large and relatively nearby Perseus Cluster of Galaxies. Wild-looking at visible wavelengths, the active galaxy is also a prodigious source of x-rays and radio emission. NGC 1275 accretes matter as entire galaxies fall into it, ultimately feeding a supermassive black hole at the galaxy's core. This color composite image made from Hubble Space Telescope data recorded during 2006. It highlights the resulting galactic debris and filaments of glowing gas, some up to 20,000 light-years long. The filaments persist in NGC 1275, even though the turmoil of galactic collisions should destroy them. What keeps the filaments together? Observations indicate that the structures, pushed out from the galaxy's center by the black hole's activity, are held together by magnetic fields. Also known as Perseus A, NGC 1275 spans over 100,000 light years and lies about 230 million light years away.
4 notes
·
View notes
Photo
Active Galaxy NGC 1275 via NASA https://ift.tt/fQ7uNj3
1 note
·
View note
Text
Oh, what's this post going to be about? A scrapped idea of mine? That's new.
I never intended to make 42 an active hunter, but before I came up with the "street vulture" lifestyle it has, I've been thinking about...a kinda weird alternative. I...somewhat wanted to connect 42 and Chester somehow for whatever reason some time ago. So I was like: "What if these two have some "symbiotic" relationships?" Although another question or, rather, questions were: "How the heck would they meet? How wouldn't one just become prey for another? How would the hippie man get the meat for 42, while the doppel gave him its protection, because, again, 42 would find Chester curious later on?"
Pinwheel Galaxy
I remember the thought of one Youtuber: "What If he (Chester) is some sort of a doppelganger as well?" But Nacho confirmed he's actually a human. The developer also said something like: "He may or may not be a time traveller". So Chester, probably, wouldn't need that from 42.
Then there's the Nightmare mode, where both are present, with Chester becoming a Nightmare version of himself. Although he seems to behave as usual. He just has tougher questions. And 42...
NGC 2207 (left) and IC 2163 (right) - the colliding spiral galaxies.
...well, I'm yet to think what it is doing there, being a VIP. I heard a thing that, apparently, people cannot dream about the things or entities which they didn't see in reality. Yet 42 doesn't really pay doormen a visit. What if it spaces out because its own mind goes to whoever is "playing" the mode and has it as a VIP? I still don't know what it'd be doing there and why, though...
NGC 1275 or Perseus A Galaxy
Another "if you read up to this point" fact:
I once thought of making a Chester blog, but I wasn't too confident about it. Maybe, it's temporary, maybe not, but, again, I'm spilling my thoughts. At least gradually, piece by piece. Even if they may not be understood by anyone, including me.
1 note
·
View note
Photo
Active Galaxy NGC 1275
0 notes
Text
Active Galaxy NGC 1275
'Active Galaxy NGC 1275' image from the #NASA_App
0 notes
Photo
Hubble Remix: Active Galaxy NGC 1275
Credits: Hubble Legacy Archive, ESA, NASA, Al Kelly
29 notes
·
View notes
Text
APOD: Active Galaxy NGC 1275 (1/26/23) Active galaxy NGC 1275 is the central, dominant member of the large and relatively nearby Perseus Cluster of Galaxies. Wild-looking at visible wavelengths, the active galaxy is also a prodigious source of x-rays and radio emission. NGC 1275 accretes matter as entire galaxies fall into it, ultimately feeding a supermassive black hole at the galaxy's core. This color composite image made from Hubble Space Telescope data recorded during 2006. It highlights the resulting galactic debris and filaments of glowing gas, some up to 20,000 light-years long. The filaments persist in NGC 1275, even though the turmoil of galactic collisions should destroy them. What keeps the filaments together? Observations indicate that the structures, pushed out from the galaxy's center by the black hole's activity, are held together by magnetic fields. Also known as Perseus A, NGC 1275 spans over 100,000 light years and lies about 230 million light years away.
0 notes