Coma Cluster
<templatestyles src="Module:Hatnote/styles.css"></templatestyles>
Coma Cluster | |
---|---|
A Sloan Digital Sky Survey/Spitzer Space Telescope mosaic of the Coma Cluster in long-wavelength infrared (red), short-wavelength infrared (green), and visible light. The many faint green smudges are dwarf galaxies in the cluster.
Credit: NASA/JPL-Caltech/GSFC/SDSS |
|
Observation data (Epoch J2000) | |
Constellation(s) | Coma Berenices |
Right ascension | 12h 59m 49s[1] |
Declination | +27° 58′ 50″[1] |
Brightest member | NGC 4874 and NGC 4889 |
Number of galaxies | > 1000[2][3] |
Richness class | 2[4] |
Bautz-Morgan classification | II [4] |
Velocity dispersion | 1,000 km/s[5] |
Redshift | 0.0231 (6 925 km/s)[1] |
Distance (co-moving) |
102 Mpc (333 Mly) h−1 0.705 [1] |
ICM temperature | 8-9 keV[6] |
Binding mass | ~7×1014[7] M☉ |
X-ray flux | (319.20 ± 2.6%)×10−12 erg s−1 cm−2[1] (0.1-2.4 keV)[1] |
Other designations | |
Abell 1656[1] | |
See also: Galaxy groups, Galaxy clusters, List of galaxy clusters | |
The Coma Cluster (Abell 1656) is a large cluster of galaxies that contains over 1,000 identified galaxies.[2][3] Along with the Leo Cluster (Abell 1367), it is one of the two major clusters comprising the Coma Supercluster.[8] It is located in and takes its name from the constellation Coma Berenices.
The cluster's mean distance from Earth is 99 Mpc (321 million light years).[3][9][10] Its ten brightest spiral galaxies have apparent magnitudes of 12–14 that are observable with amateur telescopes larger than 20 cm.[11] The central region is dominated by two supergiant elliptical galaxies: NGC 4874 and NGC 4889.[12] The cluster is within a few degrees of the north galactic pole on the sky. Most of the galaxies that inhabit the central portion of the Coma Cluster are ellipticals. Both dwarf and giant ellipticals are found in abundance in the Coma Cluster.[13]
Contents
Cluster members
As is usual for clusters of this richness, the galaxies are overwhelmingly elliptical and S0 galaxies, with only a few spirals of younger age, and many of them probably near the outskirts of the cluster.
The full extent of the cluster was not understood until it was more thoroughly studied in the 1950s by astronomers at Mount Palomar Observatory, although many of the individual galaxies in the cluster had been identified previously.[14][15][16]
Dark matter
The Coma Cluster is one of the first places where observed gravitational anomalies were considered to be indicative of unobserved mass. In 1933 Fritz Zwicky showed that the galaxies of the Coma Cluster were moving too fast for the cluster to be bound together by the visible matter of its galaxies. Though the idea of dark matter would not be accepted for another fifty years, Zwicky even wrote that the galaxies must be held together by some dunkle Materie.[17]
About 90% of the mass of the Coma cluster is believed to be in the form of dark matter. However, the distribution of dark matter throughout the cluster is poorly constrained.[18]
X-ray source
An extended X-ray source centered at 1300+28 in the direction of the Coma cluster of galaxies was reported before August 1966.[19] This X-ray observation was performed by balloon, but the source was not detected in the sounding rocket flight launched by the X-ray astronomy group at the Naval Research Laboratory on November 25, 1964.[20] A strong X-ray source was observed by the X-ray observatory satellite Uhuru close to the center of the Coma cluster and this source was suggested be designated Coma X-1.[21]
The Coma cluster contains about 800 galaxies within a 100 x 100 arc-min area of the celestial sphere. The source near the center at RA (1950) 12h56m ± 2m Dec 28°6' ± 12' has a luminosity Lx = 2.6 x 1044 ergs/s.[21] As the source is extended, with a size of about 45', this argues against the possibility that a single galaxy is responsible for the emission.[21] The Uhuru observations indicated a source strength of no greater than ~10−3 photons cm−2s−1keV−1 at 25 keV,[21] which disagrees with the earlier observations[19] claiming a source strength of ~10−2 photons cm−2s−1keV−1 at 25 keV, and a size of 5°.
Gallery
-
Hubble close-up on the Coma Cluster.jpg
Hubble close-up on the Coma Cluster.[22]
-
NGC 4911.jpg
A majestic face-on spiral galaxy (NGC 4911) located deep within the Coma Cluster.
-
ComaGalaxy.jpg
Coma Cluster photographed through 8" Celestron Edge HD in San Diego, CA.[23]
-
Comacl zentrum600.png
Map of the central part of the Coma Cluster.
See also
- List of galaxy groups and clusters
- Eridanus Cluster
- Fornax Cluster – another nearby cluster of galaxies
- Norma Cluster
- Virgo Cluster – another nearby cluster of galaxies
- X-1 X-ray source
References
<templatestyles src="Reflist/styles.css" />
Cite error: Invalid <references>
tag; parameter "group" is allowed only.
<references />
, or <references group="..." />
External links
- The Coma Cluster of Galaxies - Astronomy Picture of the Day, NASA, 2000 August 6
- The dynamical state of the Coma cluster with XMM-Newton
- Very Small Array observations of the Sunyaev-Zel'dovich effect in nearby galaxy clusters
- Hubble Space Telescope Treasury Survey of the Coma Cluster
- The Coma Cluster on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Coordinates: 12h 59m 49s, +27° 58′ 50″
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 Lua error in package.lua at line 80: module 'strict' not found. Chandra/Field Guide to X-ray Sources: Coma Cluster at the Wayback Machine (archived February 21, 2008)
- ↑ 3.0 3.1 3.2 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 4.0 4.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Section 4 of Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Newswise: Hubble's Sweeping View of the Coma Cluster of Galaxies Retrieved on June 11, 2008.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 19.0 19.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 21.0 21.1 21.2 21.3 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ http://www.astrobin.com/244071/