Antlia Dwarf

Antlia Dwarf

Antlia Dwarf by Hubble space telescope
Observation data (J2000 epoch)
Constellation Antlia
Right ascension 10h 04m 03.9s[1]
Declination −27° 19′ 55″[1]
Redshift 362 ± 0 km/s[1]
Distance 1.32 ± 0.06[2]Mpc
1.33 ± 0.10[3] Mpc
1.31 ± 0.03[4] Mpc
1.29 ± 0.02[5] Mpc
1.25[6] Mpc
Group or cluster Antlia Group
Type dE3.5[1] dSph,[3] dSph/Irr
Mass 3 × 107 M☉
Apparent dimensions (V) 2′.0 × 1′.5[1]
Apparent magnitude (V) 15.67 ± 0.02[2]
Other designations
Antlia Dwarf Galaxy,[1] PGC 29194[1]

The Antlia Dwarf is a dwarf spheroidal/irregular galaxy. It lies about 1.3 Mpc (4.3 million light-years) from Earth in the constellation Antlia. It is the fourth and faintest member of the nearby Antlia Group of galaxies. The galaxy contains stars of all ages, contains significant amounts of gas, and has experienced recent star formation. The Antlia Dwarf is believed to be tidally interacting with the small barred spiral galaxy, NGC 3109.[3][7]

Discovery

Antlia Dwarf was first cataloged in 1985 by H. Corwin, Gérard de Vaucouleurs, and A. de Vaucouleurs. Later in 1985 and 1987 it was noted as a possible nearby dwarf galaxy by two groups of astronomers.[3] It was finally confirmed as a dwarf galaxy in 1997 by Alan Whiting, Mike Irwin and George Hau during a survey of the northern sky. They for the first time resolved it into stars and determined the distance to it—1.15 Mpc (the modern distance estimate is slightly larger).[8]

In 1999 Antlia Dwarf was identified by Sidney van den Bergh as the fourth member of the Antlia Group—the group of galaxies closest to the Local Group.[3]

Properties

The Antlia Dwarf is classified alternatively as a dwarf elliptical galaxy of type dE3.5,[8][9] or either as a dwarf spheroidal galaxy (dSph) or as a transitional galaxy from spheroidal to irregular types (dSph/Irr).[3] The last classification is due to a substantial star formation in this galaxy in the last 0.1 billion years.

Antlia Dwarf comprises two components: a core and an old halo.[2] Its half-light radius is about 0.25 kpc.[8] The metallicity is very low, at about <[Fe/H]>=−1.6 to −1.9 meaning that Antlia Dwarf contains 40–80 times less heavy elements than the Sun.[2][10] The galaxy has a well-defined and easily observed red giant branch, which makes measuring its distance relatively easy.[9] The total luminosity of Antlia Dwarf is approximately 1 million that of the Sun (the visible absolute magnitude is MV=−10.3).[2]

The stellar mass of Antlia Dwarf is estimated to be about 2–4×106 solar masses, while its total mass (within the visible radius) is approximately 4 × 107 solar masses.[2] The galaxy contains stars of all ages but is dominated by old stars with the age of more than 10 billion year. There seems to have been a major episode of star formation in the Antlia Dwarf around 100 million years ago.[4][9] However, the young stars are confined to the central core of the galaxy.[10]

Antlia Dwarf is unusual among dwarf spheroidal galaxies in that it contains large amounts (as much as 7 ×105 solar masses) of neutral atomic hydrogen.[11][12] However it does not have significant H II regions and does not actively form stars at the present moment.[9]

Location and interactions

The Antlia Dwarf is located about 1.31 megaparsecs (4.3×10^6 ly) away, in the constellation Antlia.[9] Its distance from the barycenter of the Local Group is about 1.7 Mpc. At this distance, it is situated well outside the Local Group and is a member of a separate group of dwarf galaxies called Antlia Group.[3] The Antlia Dwarf is separated from the small spiral/irregular galaxy NGC 3109 by only 1.18 degrees on the sky, which corresponds to a physical separation of 29 kiloparsecs (95×10^3 ly) to 180 kiloparsecs (590×10^3 ly) depending on their radial separation.[3][2]

The Antlia Dwarf and NGC 3109 may be actually physically bound if the distance between them is not very large.[3][8] However their velocity relative to each other—43 km/s[3] makes it questionable whether they are in fact a bound system, especially if the distance between them is closer to the upper limit—180 kpc.[2][9] If they are gravitationally bound, their total mass may be as high as 78 billion solar masses.[4]

Observations have also demonstrated that NGC 3109 has a warp in its gaseous disk that is traveling at the same velocity as the gas in the Antlia Dwarf, indicating that the two galaxies had a close encounter about one billion years ago.[12]

References

  1. 1 2 3 4 5 6 7 "NASA/IPAC Extragalactic Database". Results for Antlia Dwarf. Retrieved 30 November 2006.
  2. 1 2 3 4 5 6 7 8 Aparicio, A.; Dalcanton, J. J.; Gallart, C.; Martinez-Delgado, D. (October 1997). "The Nature of the Antlia Galaxy: A New Dwarf Irregular in the Outskirts of the Local Group.". The Astronomical Journal 114 (4): 1447–1457. Bibcode:1997AJ....114.1447A. doi:10.1086/118575.
  3. 1 2 3 4 5 6 7 8 9 10 Van Den Bergh, S. (1999). "The Nearest Group of Galaxies". The Astrophysical Journal 517 (2): L97. arXiv:astro-ph/9904425. Bibcode:1999ApJ...517L..97V. doi:10.1086/312044.
  4. 1 2 3 Piersimoni, A. M.; Piersimoni, A. M.; Bono, G.; Castellani, M.; Marconi, G.; Cassisi, S.; Buonanno, R.; Nonino, M. (December 1999). "A new investigation on the Antlia Dwarf Galaxy". Astronomy and Astrophysics 352: L63–L68. arXiv:astro-ph/9909198. Bibcode:1999A&A...352L..63P.
  5. ↑ Dalcanton, J. J.; Williams, B. F.; Seth, A. C.; Dolphin, A.; Holtzman, J.; Rosema, K.; Skillman, E. D.; Cole, A.; Girardi, L. O.; Gogarten, S. M.; Karachentsev, I. D.; Olsen, K.; Weisz, D.; Christensen, C.; Freeman, K.; Gilbert, K.; Gallart, C.; Harris, J.; Hodge, P.; De Jong, R. S.; Karachentseva, V.; Mateo, M.; Stetson, P. B.; Tavarez, M.; Zaritsky, D.; Governato, F.; Quinn, T. (2009). "The Acs Nearby Galaxy Survey Treasury". The Astrophysical Journal Supplement Series 183: 67. arXiv:0905.3737. Bibcode:2009ApJS..183...67D. doi:10.1088/0067-0049/183/1/67.
  6. ↑ Tully, R. B.; Rizzi, L.; Dolphin, A. E.; Karachentsev, I. D.; Karachentseva, V. E.; Makarov, D. I.; Makarova, L.; Sakai, S.; Shaya, E. J. (2006). "Associations of Dwarf Galaxies". The Astronomical Journal 132 (2): 729. arXiv:astro-ph/0603380. Bibcode:2006AJ....132..729T. doi:10.1086/505466.
  7. ↑ Grebel, Eva K.; Gallagher, John S., III; Harbeck, Daniel (April 2003). "The Progenitors of Dwarf Spheroidal Galaxies". The Astronomical Journal 125 (4): 1926–1939. arXiv:astro-ph/0301025. Bibcode:2003AJ....125.1926G. doi:10.1086/368363.
  8. 1 2 3 4 Whiting, Alan B.; Irwin, M. J.; Hau, George K. T. (September 1997). "A new galaxy in the Local Group: The Antlia Dwarf Galaxy". The Astronomical Journal 114 (3): 996–1001. arXiv:astro-ph/9706173. Bibcode:1997AJ....114..996W. doi:10.1086/118530.
  9. 1 2 3 4 5 6 Pimbblet, K. A.; Couch, W. J. (2011). "Antlia Dwarf Galaxy: Distance, quantitative morphology and recent formation history via statistical field correction". Monthly Notices of the Royal Astronomical Society 419 (2): 1153. arXiv:1109.1142. Bibcode:2012MNRAS.419.1153P. doi:10.1111/j.1365-2966.2011.19769.x.
  10. 1 2 Sarajedini, Ata; Claver, C. F.; Ostheimer, James C. Jnr.; Ostheimer, James C. (December 1997). "The properties of the Antlia Dwarf Galaxy". The Astronomical Journal 114 (6): 2505–2513. Bibcode:1997AJ....114.2505S. doi:10.1086/118663.
  11. ↑ van den Bergh, Sidney (2000). The galaxies of the Local Group. University of Cambridge. p. 266. ISBN 0-521-65181-6.
  12. 1 2 Barnes, D. G.; W. J. G. de Blok (August 2001). "On the Neutral Gas Content and Environment of NGC 3109 and the Antlia Dwarf Galaxy". The Astronomical Journal 122 (2): 825. arXiv:astro-ph/0107474. Bibcode:2001AJ....122..825B. doi:10.1086/321170. Retrieved 24 September 2010.

External links

Coordinates: 10h 04m 03.9s, −27° 19′ 55″

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