Astronomy:Laevens 1
Coordinates: 
11h 36m 16.5s, −10° 52′ 37.1″
| Laevens 1 | |
|---|---|
 Laevens 1 | |
| Observation data (J2000 epoch) | |
| Constellation | Crater |
| Right ascension | 11h 36m 16.2s[1] |
| Declination | –10° 52′ 38.8″[1] |
| Distance | 145 kiloparsecs (470 kly)[2] |
| Apparent dimensions (V) | 0.46 arcmins[3] |
| Physical characteristics | |
| Absolute magnitude | −5.3[2] |
| Mass | 1×104[2] M☉ |
| Radius | 50 parsecs (160 ly)[3] |
| VHB | 14.2 |
| Metallicity | [math]\displaystyle{ \begin{smallmatrix}\left[\ce{Fe}/\ce{H}\right]\end{smallmatrix} }[/math] = –1.65[2] dex |
| Estimated age | 7.5 Gyr[2] |
| Notable features | Unusually young and distant Milky way cluster. |
| Other designations | Crater cluster, PSO J174.0675-10.8774 |
Laevens 1 is a faint globular cluster in the constellation Crater that was discovered in 2014. It is also known as Crater, the Crater cluster and PSO J174.0675-10.8774.
At a distance of 145 kiloparsecs (470 kly) it is the most distant Milky Way globular cluster yet known, located in the galactic halo surrounding the Milky Way galaxy.[1] With an age of only 7.5 Gyr, it is likely to have been incorporated into our galaxy long after the formation of the Milky Way, probably during an interaction with the Small Magellanic Cloud.[2][4][5]
Some analyses initially categorized it as a satellite galaxy, because of the presence of a handful of blue loop stars and a sparsely populated red clump; the existence of some of these types of stars in Laevens 1 would imply relatively recent star formation (within 400 Myr). Such recent formation would be very atypical for a globular cluster;[6] more recent work suggests that some of these stars were erroneously assigned membership of the cluster, distorting the overall result. After removing these, the subsequent reanalysis concluded that Laevens 1 is a faint, intermediate-age globular cluster.[7]
Laevens 1 is orbiting the galaxy at approximately the same distance as the ultrafaint dwarf galaxies Leo IV and Leo V. This hints that all three satellites may once have been closely associated before falling together into the Milky Way halo.[6]
See also
References
- ↑ 1.0 1.1 1.2 Laevens, Benjamin P. M.; Martin, Nicolas F.; Sesar, Branimir; Bernard, Edouard J.; Rix, Hans-Walter; Slater, Colin T.; Bell, Eric F.; Ferguson, Annette M. N. et al. (2014-05-01). "A New Distant Milky Way Globular Cluster in the Pan-STARRS1 3pi Survey". The Astrophysical Journal Letters 786 (1): L3. doi:10.1088/2041-8205/786/1/L3. ISSN 0004-637X. Bibcode: 2014ApJ...786L...3L.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Weisz, Daniel R.; Koposov, Sergey E.; Dolphin, Andrew E.; Belokurov, Vasily; Gieles, Mark; Mateo, Mario L.; Olszewski, Edward W.; Sills, Alison et al. (2015-10-28). "A Hubble Space Telescope Study of the Enigmatic Milky Way Halo Globular Cluster Crater". The Astrophysical Journal 822 (1): 32. doi:10.3847/0004-637X/822/1/32. Bibcode: 2016ApJ...822...32W.
- ↑ 3.0 3.1 effective radius
- ↑ "Thieving Milky Way stole distant star cluster from neighbour". New Scientist. 2015-11-19. https://www.newscientist.com/article/dn28519-thieving-milky-way-stole-distant-star-cluster-from-neighbour/. Retrieved 2016-01-26.
- ↑ Kirby, Evan N.; Simon, Joshua D.; Cohen, Judith G. (2015-01-01). "Spectroscopic Confirmation of the Dwarf Galaxies Hydra II and Pisces II and the Globular Cluster Laevens 1". The Astrophysical Journal 810 (1): 56. doi:10.1088/0004-637X/810/1/56. ISSN 0004-637X. Bibcode: 2015ApJ...810...56K. http://stacks.iop.org/0004-637X/810/i=1/a=56.
- ↑ 6.0 6.1 Belokurov, V.; Irwin, M. J.; Koposov, S. E.; Evans, N. W.; Gonzalez-Solares, E.; Metcalfe, N.; Shanks, T. (2014-07-01). "ATLAS lifts the Cup: discovery of a new Milky Way satellite in Crater". Monthly Notices of the Royal Astronomical Society 441 (3): 2124–2133. doi:10.1093/mnras/stu626. ISSN 0035-8711. Bibcode: 2014MNRAS.441.2124B.
- ↑ Voggel, Karina; Hilker, Michael; Baumgardt, Holger; Collins, Michelle L.M.; Grebel, Eva K.; Husemann, Bernd; Richtler, Tom; Frank, Matthias J. (2016). "Probing the boundary between star clusters and dwarf galaxies: A MUSE view on the dynamics of Crater/Laevens I". Monthly Notices of the Royal Astronomical Society 460 (3): 3384–3397. doi:10.1093/mnras/stw1132. Bibcode: 2016MNRAS.460.3384V.
External links
- "NAME Laevens 1". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NAME+Laevens+1.
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