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Andromeda XXI

From Wikipedia, the free encyclopedia
Dwarf spheroidal galaxy in constellation Andromeda
"Andromeda 21" redirects here. For the star, see21 Andromedae.
Andromeda XXI
Observation data (J2000epoch)
ConstellationAndromeda
Right ascension23h 54m 47.7s[1]
Declination+42° 28′ 15″[1]
Distance859 ± 51 kiloparsecs (2.80 ± 0.17 Mly)[2]
Apparent magnitude (V)15.5 ± 0.3[3]
Absolute magnitude (V)−9.1 ± 0.3[3]
Characteristics
TypedSph
Half-light radius (physical)1005±175 pc[3]
Half-light radius (apparent)4.1+0.8
−0.4
[3]
Notable featuresSatellite galaxy
ofAndromeda
Other designations
Andromeda XXI, And XXI, And 21

Andromeda XXI (And 21,And XXI) is a moderately brightdwarf spheroidal galaxy about 859 ± 51 kiloparsecs (2.80 ± 0.17 Mly) away from theSun in theconstellationAndromeda. It is the fourth largestLocal Group dwarf spheroidal galaxy. The discovery arose from the first year data of aphotometric survey of theM31/M33 subgroupings of the Local Group by thePan-Andromeda Archaeological Survey (PAndAS). This survey was conducted with the Megaprime/MegaCam wide-field camera mounted on theCanada-France-Hawaii Telescope.

This largesatellite of theAndromeda Galaxy (M31) has a half-light radius of roughly 1 kpc.[2]

Andromeda XXI appears as a spatial overdensity of stars. It has red giant branches at the distance of M31/M33, and follows metal-poor, [Fe/H]=-1.8 when plotted in a color-magnitude diagram.

Like other dwarf spheroidal galaxies, Andromeda XXI shows no sign of currentstar formation and appears to have had 90% of its stars formed 5.8 billion years ago.[3] Its centraldark matter density is lower than expected from theΛCDM model, but this could be explained if it lost most of its mass in a previoustidal stripping event or had experience tidal shocks from an eccentric orbit.[3]

Although moderately bright (MV = −9.1 ± 0.3),[3] it has lowsurface brightness. This indicates that numerous relatively luminous M31 satellites remain undiscovered.

See also

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References

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  1. ^ab"NAME Andromeda XXI".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2 April 2011.
  2. ^abNicolas F. Martin, Alan W. McConnachie, Mike Irwin, Lawrence M. Widrow, Annette M. N. Ferguson, Rodrigo A. Ibata, John Dubinski, Arif Babul, Scott Chapman, Mark Fardal, Geraint F. Lewis, Julio Navarro, R. Michael Rich;"PAndAS' cubs: discovery of two new dwarf galaxies in the surroundings of the Andromeda and Triangulum galaxies";The Astrophysical Journal, Volume 705, Issue 1, pp. 758-765 (2009);doi:10.1088/0004-637X/705/1/758;Bibcode:2009ApJ...705..758M;arXiv:0909.0399;
  3. ^abcdefgCollins, Michelle L M.; Read, Justin I.; Ibata, Rodrigo A.; Rich, R Michael; Martin, Nicolas F.; Peñarrubia, Jorge; Chapman, Scott C.; Tollerud, Erik J.; Weisz, Daniel R. (2021)."Andromeda XXI – a dwarf galaxy in a low-density dark matter halo".Monthly Notices of the Royal Astronomical Society.505 (4):5686–5701.arXiv:2102.11890.doi:10.1093/mnras/stab1624.
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