Misplaced Pages

Phoenix Dwarf: Difference between revisions

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Browse history interactively← Previous editNext edit →Content deleted Content addedVisualWikitext
Revision as of 03:52, 29 July 2017 editGraeme Bartlett (talk | contribs)Administrators249,578 edits discussion at Misplaced Pages talk:WikiProject Astronomy#CMG - "Catalogue of One Thousand Named Galaxies" decides not to include← Previous edit Revision as of 20:40, 27 February 2018 edit undoTom.Reding (talk | contribs)Autopatrolled, Extended confirmed users, Page movers, Template editors3,801,455 editsm Fix Category:Pages using deprecated image syntax; WP:GenFixes on, using AWBNext edit →
Line 1: Line 1:
{{Infobox Galaxy {{Infobox Galaxy
| image = ] | image = Phoenix Dwarf Hubble WikiSky.jpg
| image_size = 300px
| caption= Phoenix Dwarf by the ] | caption= Phoenix Dwarf by the ]
| name = Phoenix Dwarf Galaxy | name = Phoenix Dwarf Galaxy
Line 67: Line 68:


== Characteristics == == Characteristics ==
The Phoenix Dwarf has an inner part of young ]s which is stretched in an east-west direction and an outer part of mainly old stars that is stretched north-south. The central region's rate of ] seems to have been relatively constant across time (Martínez-Delgado et al. 1999). In 1999, St-Germain et al. discovered a ] region of about 10<sup>5</sup> {{Solar mass|link=y}} just to the west of Phoenix. Its ] is -23&nbsp;km/s and may be physically associated with Phoenix if it is found to have a similar radial velocity.<ref name="Bergh2000">{{ Cite journal The Phoenix Dwarf has an inner part of young ]s which is stretched in an east-west direction and an outer part of mainly old stars that is stretched north-south. The central region's rate of ] seems to have been relatively constant across time (Martínez-Delgado et al. 1999). In 1999, St-Germain et al. discovered a ] region of about 10<sup>5</sup> {{Solar mass|link=y}} just to the west of Phoenix. Its ] is -23&nbsp;km/s and may be physically associated with Phoenix if it is found to have a similar radial velocity.<ref name="Bergh2000">{{Cite journal
| last1 = van den Bergh | last1 = van den Bergh
| first1 = Sidney | first1 = Sidney

Revision as of 20:40, 27 February 2018

Phoenix Dwarf Galaxy
Phoenix Dwarf by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationPhoenix
Right ascension01 51 06.3
Declination−44° 26′ 41″
Redshift60 ± 30 km/s
Distance1.44 ± 0.07 Mly (440 ± 20 kpc)
Apparent magnitude (V)13.1
Characteristics
TypeIAm
Apparent size (V)4′.9 × 4′.1
Notable features-
Other designations
ESO 245- G 007, PGC 6830

The Phoenix Dwarf is a dwarf irregular galaxy discovered in 1976 by Hans-Emil Schuster and Richard Martin West and mistaken for a globular cluster. It is currently 1.44 Mly away from Earth. Its name comes from the fact that it is part of the Phoenix constellation.

Characteristics

The Phoenix Dwarf has an inner part of young stars which is stretched in an east-west direction and an outer part of mainly old stars that is stretched north-south. The central region's rate of star formation seems to have been relatively constant across time (Martínez-Delgado et al. 1999). In 1999, St-Germain et al. discovered a H I region of about 10 M just to the west of Phoenix. Its radial velocity is -23 km/s and may be physically associated with Phoenix if it is found to have a similar radial velocity.

References

  1. ^ "NASA/IPAC Extragalactic Database". Results for Phoenix Dwarf. Retrieved 2007-03-15.
  2. I. D. Karachentsev; V. E. Karachentseva; W. K. Hutchmeier; D. I. Makarov (2004). "A Catalog of Neighboring Galaxies". Astronomical Journal. 127 (4): 2031–2068. Bibcode:2004AJ....127.2031K. doi:10.1086/382905.
  3. Karachentsev, I. D.; Kashibadze, O. G. (2006). "Masses of the local group and of the M81 group estimated from distortions in the local velocity field". Astrophysics. 49 (1): 3–18. Bibcode:2006Ap.....49....3K. doi:10.1007/s10511-006-0002-6.
  4. Schuster, H.-E.; West, R. M. (May 1976). "A very distant globular cluster?". Astronomy & Astrophysics. 49: 129–131. Bibcode:1976A&A....49..129S.
  5. Canterna, R.; Flower, P. J. (March 1977). "A new dwarf irregular galaxy in the constellation Phoenix". Astrophysical Journal. 212 (Letters): L57–L58. Bibcode:1977ApJ...212L..57C. doi:10.1086/182374.
  6. van den Bergh, Sidney (April 2000). "Updated Information on the Local Group". The Publications of the Astronomical Society of the Pacific. 112 (770): 529–536. arXiv:astro-ph/0001040. Bibcode:2000PASP..112..529V. doi:10.1086/316548.

External links


Milky Way
LocationMilky Way → Milky Way subgroup → Local GroupLocal SheetVirgo SuperclusterLaniakea Supercluster → Local Hole → Observable universe → Universe
Each arrow (→) may be read as "within" or "part of".
The Milky Way Galaxy
The Milky Way Galaxy
Structure
Galactic Center
Disk
Halo
Satellite
galaxies
Magellanic Clouds
Dwarfs
Related
Categories: