Fornax Cluster Explained

Fornax Cluster should not be confused with Furneaux Group.

The Fornax Cluster is a cluster of galaxies lying at a distance of 19 megaparsecs (62 million light-years).[1] It has an estimated mass of solar masses,[2] making it the second richest galaxy cluster within 100 million light-years, after the considerably larger Virgo Cluster. It may be associated with the nearby Eridanus Group. It lies primarily in the constellation Fornax, with its southern boundaries partially crossing into the constellation of Eridanus, and covers an area of sky about 6° across or about 28 sq degrees.

The Fornax Cluster is a particularly valuable source of information about the evolution of such clusters due to its relatively close proximity to the Sun. It also shows the gravitational effects of a merger of a galaxy subgroup with the main galaxy group,[3] which in turn lends clues about the associated galactic superstructure.[4] At the centre of the cluster lies NGC 1399. Other cluster members include NGC 1316 (the group's brightest galaxy), NGC 1365, NGC 1427A, NGC 1427 and NGC 1404.

Structure

Fornax can be divided into two subclusters: the main cluster, centered on NGC 1399, and a subgroup 3 degrees to the southwest centered on the lenticular galaxy NGC 1316 that is currently in the process of infalling with the largest subcluster to merge with it, and whose galaxies are experiencing relatively strong star formation activity. [5]

Intracluster medium

As with many other galaxy clusters, Fornax intracluster medium is filled with a hot, rarefied gas that emits X-rays.[6] and contains a number of intergalactic stars, some of which have produced novae.[7]

List of cluster members

Designation! colspan="2"
Coordinates (Epoch 2000)TypeMean Angular diameter
(arcminutes)
Diameter
(x1000 Light-years)
Distance
(mly)
Recessional velocity
(km/s)
Right AscensionDeclination
ESO 357-0703 10.4−33 0914.7SBm2.2 40981
ESO 357-1203 16.9−35 3214.8SBcd2.2 401445
03 19.6−32 2814.5SBb2.1 40671318
03 21.1−37 0613 SBc1.9 3564 1640
03 22.1−37 35? Irr2.9 551507
03 22.7−37 129.4 (R')SAB(s)011.5215621664
03 22.7−37 0611.9SBa3.0 5570 1935
03 23.9−36 2811.5S04.3 8063 1247
NGC 1326A03 25.1−36 2214.7SBm1.7 30841719
NGC 1326B03 25.3−36 2313.7SBm3.5 6546888
03 26.0−32 5413.9E1.6 30611158
03 26.5−35 4313.4E1.9 35651360
03 28.0−37 0913.3SBab1.6 30861760
03 28.1−32 1712.8E1.9 35641240
03 28.3−31 0411.2E5.6 105601052
03 28.8−35 1114.2SBbc2.3 451241
ESO 358-1003 29.7−33 3314.8E1.5 301620
03 30.6−34 5112.4E-S03.2 6069 1420
NGC 135003 31.1−33 3811.2Sa(r)5.8 13087 1905
03 33.6−36 0810.3(R')SBb(s)b11.020556 1636
03 33.9−31 1213.1S01.9 35561137
03 35.3−35 1411.0E2.7 5059 1240
NGC 137503 35.3−35 1612.2SB0 pec2.1 2328 643
03 35.5−34 2713.4S02.3 4560 1530
03 36.1−35 2611.9E2.6 50601264
03 36.5−34 599.9S04.8 8560 1737
03 36.5−35 1811.5S02.6 5560 1673
03 36.8−36 1513.6Sa1.7 30651340
03 36.8−36 0011.2(R)SA(r)0/a3.4 6553 868
03 36.8−34 4413.4S02.5 45721419
03 37.0−35 3010.8(R')SAB(s)03.2 6053 1296
03 37.1−35 1213.8E1.5 30801697
03 37.2−35 4512.6E2.6 5042 883
03 38.6−35 2713.8E0.7 767 853
03 38.5−35 269.9E6.8 13066 1335
03 38.9−35 3610.9E4.1 7565 1942
03 39.4−31 1912.9SBbc3.9 7550963
03 40.1−35 3813.4Irr2.1 4052 2028
ESO 358-5003 41.1−33 4713.9S01.6 301151
ESO 358-5103 41.5−34 5314.1Sa1.5 301626
03 42.2−29 5411.4SA(rs)b6.0 11569 1402
03 42.3−35 2411.8E3.6 7071 1327
03 42.4−35 0914.0E1.5 3075 1602
NGC 1437A03 43.0−36 1614.2SBd1.7 3041798
03 43.6−35 5111.7SBab2.8 5058 1296
ESO 358-6003 45.2−35 3415.6Irr1.7 30710
NGC 1437B03 45.9−36 2214.0Sc2.5 45691415
03 46.2−36 4213.5SB01.7 3063 1341
PGC 1380903 46.3−34 5712.6Sc4.8 901838
03 47.1−33 4212.6(R')SA(s)bc2.5 4550 1057
ESO 302-0903 47.6−38 3514.6SBd2.2 40908
ESO 302-1403 51.7−38 2715.5Irr1.5 30798
ESO 359-0303 52.0−33 2814.1Sab1.8 351495
03 54.3−36 5813.9Sb2.5 4548952
03 54.3−35 5812.5E1.9 3565 1382
04 11.2−32 5112.9S01.3 15 57 1169
04 12.1−32 5210.7SBb12.6 210 57
(*) - Membership is uncertain

See also

Notes and References

  1. Jordán . A. . Blakeslee . J. P. . Côté . P. . Ferrarese . L. . Infante . L. . Mei . S. . Merritt . D. . David Merritt . Peng . E. W. . Tonry . J. . West . Michael J. . June 2006 . The Astrophysical Journal Supplement Series . 452 . 1 . 141–153 . The ACS Fornax Cluster Survey. I. Introduction to the Survey and Data Reduction Procedures . 2007ApJS..169..213J . 10.1086/512778 . astro-ph/0702320 . 17845709 . 8 .
  2. Drinkwater. Michael J.. Gregg. Michael D.. Colless. Matthew. 2001-02-01. Substructure and Dynamics of the Fornax Cluster. The Astrophysical Journal Letters. 548. 2 . L139–L142. 10.1086/319113. astro-ph/0012415 . 2001ApJ...548L.139D . 13456590 . 0004-637X.
  3. Web site: Hubble Heritage Project. Dwarf Irregulars and Galaxy Clusters. 2006-12-07.
  4. Web site: Chandra X-Ray Observatory. Fornax Cluster: Motions of Nearby Galaxy Cluster Reveal Presence of Hidden Superstructure. 2006-12-07.
  5. Drinkwater. Michael J.. Gregg. Michael D.. Colless. Matthew. February 2001. The Astrophysical Journal Letters. 548. 2. L139. Substructure and Dynamics of the Fornax Cluster . 10.1086/319113. astro-ph/0012415. 2001ApJ...548L.139D . 13456590.
  6. Web site: Fornax Cluster: Motions of Nearby Galaxy Cluster Reveal Presence of Hidden Superstructure . NASA . 30 April 2005 . 10 December 2012.
  7. Neill. James D.. Shara. Michael M.. Oegerle. William R.. January 2005. The Astrophysical Journal. 618. 2. 692–704. Tramp Novae between Galaxies in the Fornax Cluster: Tracers of Intracluster Light. astro-ph/0409265 . 2005ApJ...618..692N . 10.1086/426049 . 5649912.