Astronomy:Pisces Overdensity
| Pisces Overdensity | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Pisces |
| Right ascension | 23h 19m 00s[1] |
| Declination | +00° 00′ 00″[1] |
| Distance | 260 kly (80 kpc)[2] |
| Absolute magnitude (V) | −10.35[3] |
| Characteristics | |
| Type | dIrr/dSph[3] |
| Apparent size (V) | ~1°[4] |
| Other designations | |
| Pisces Plume[1] | |
The Pisces Overdensity is a clump of stars in the Milky Way's halo, which may be a disrupted dwarf spheroidal galaxy.[5] It is situated in the Pisces constellation and was discovered in 2009 by analysis of distribution of RR Lyrae stars in the data obtained by the Sloan Digital Sky Survey's data.[2] The galaxy is located at the distance of about 80 kpc from the Sun and moves towards it with a speed of about 75 km/s.[4]
The Pisces Overdensity is one of the faintest satellites of the Milky Way.[5] Its mass is estimated to be at least 105 Solar masses.[2] However it has a large size of about several degrees (around 1 kpc) and may be in a transitional phase between a gravitationally bound galaxy and completely unbound system.[4] The Pisces Overdensity is located near the plane, where the Magellanic Clouds lie. There may exist a connection between the Magellanic stream and this galaxy.[2]
References
- ↑ 1.0 1.1 1.2 "NAME Pisces Overdensity". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NAME+Pisces+Overdensity.
- ↑ 2.0 2.1 2.2 2.3 Watkins, L. L. et al. (2009), "Substructure revealed by RR Lyraes in SDSS Stripe 82", Monthly Notices of the Royal Astronomical Society 398 (4): 1757–70, doi:10.1111/j.1365-2966.2009.15242.x, Bibcode: 2009MNRAS.398.1757W.
- ↑ 3.0 3.1 Boyer, Martha L; Skillman, Evan D; Van Loon, Jacco Th; Gehrz, Robert D; Woodward, Charles E (2009). "Aspitzerstudy of Asymptotic Giant Branch Stars. Iii. Dust Production and Gas Return in Local Group Dwarf Irregular Galaxies". The Astrophysical Journal 697 (2): 1993. doi:10.1088/0004-637X/697/2/1993. Bibcode: 2009ApJ...697.1993B.
- ↑ 4.0 4.1 4.2 Kollmeier, Juna A. et al. (2009), "Spectroscopic Confirmation of the Pisces Overdensity", The Astrophysical Journal Letters 705 (2): L158–L162, doi:10.1088/0004-637X/705/2/L158, Bibcode: 2009ApJ...705L.158K.
- ↑ 5.0 5.1 Belokurov, V. et al. (2010), "Big fish, small fish: Two New Ultra-Faint Satellites of the Milky Way", The Astrophysical Journal Letters 712: L103–106, doi:10.1088/2041-8205/712/1/L103, Bibcode: 2010ApJ...712L.103B.
| Location | Milky Way → Milky Way subgroup → Local Group → Local Sheet → Virgo Supercluster → Laniakea Supercluster → Observable universe → Universe Each arrow (→) may be read as "within" or "part of". |  | |||||||
|---|---|---|---|---|---|---|---|---|---|
| Galactic core | |||||||||
| Spiral arms | |||||||||
| Satellite galaxies |
| ||||||||
| Related | |||||||||
 |  |
