| Palomar 6 | |
|---|---|
 | |
| Observation data ( J2000 epoch) | |
| Class | XI |
| Constellation | Ophiuchus |
| Right ascension | 17h 43m 42.20s [1] |
| Declination | −26° 13′ 21.0″ [1] |
| Distance | 25.02 ± 0.62 kly (7.67 ± 0.19 kpc) [2] |
| Physical characteristics | |
| Mass | 2.28×105 [3] M☉ |
| Metallicity | = –0.91 [3] dex |
| Estimated age | 12.4 ± 0.9 Gyr [2] |
| Other designations | ESO 520-21, GCl 75, 1740-262 [1] |
![{\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4c0821bd80891e071c08e7c7ee8e022baedf522c)
Palomar 6 is a loose globular cluster in the constellation Ophiuchus that belongs to the Milky Way galaxy. It is a member of the Palomar Globular Clusters group. It is located about 25,000 light-years (7,700 parsecs) away from the Sun. [2] It formed in what would become the bulge of the Milky Way. It is similar to other old-bulge globular clusters such as Messier 62, NGC 6522, NGC 6558, and Haute-Provence 1. [2]
First discovered on the National Geographic Society – Palomar Observatory Sky Survey plates by Robert G. Harrington and Fritz Zwicky, [4] it was catalogued as a globular cluster, and is one of four globulars known to contain a planetary nebula.
References
- ^ a b c "SIMBAD Astronomical Database". Results for Palomar 6. Retrieved 2009-10-04.
- ^ a b c d Souza, S. O.; Valentini, M.; Barbuy, B.; Pérez-Villegas, A.; Chiappini, C.; Ortolani, S.; Nardiello, D.; Dias, B.; Anders, F.; Bica, E. (2021). "Photo-chemo-dynamical analysis and the origin of the bulge globular cluster Palomar 6". Astronomy & Astrophysics. 656: A78. arXiv: 2109.04483. doi: 10.1051/0004-6361/202141768. S2CID 237485386.
- ^ a b Boyles, J.; et al. (November 2011), "Young Radio Pulsars in Galactic Globular Clusters", The Astrophysical Journal, 742 (1): 51, arXiv: 1108.4402, Bibcode: 2011ApJ...742...51B, doi: 10.1088/0004-637X/742/1/51, S2CID 118649860.
- ^ Abell, George O. (1955). "Globular Clusters and Planetary Nebulae Discovered on the National Geographic Society-Palomar Observatory Sky Survey". Publications of the Astronomical Society of the Pacific. 67 (397): 258. Bibcode: 1955PASP...67..258A. doi: 10.1086/126815.
External links
-
Media related to
Palomar 6 at Wikimedia Commons - Simbad reference data
- SEDS: Palomar 6, Capricornus Dwarf
- Palomar 6 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- NASA Astronomy Picture of the Day: Palomar 6: Globular Star Cluster (19 October 2021)
 | This star cluster–related article is a stub. You can help Wikipedia by expanding it. |
| Palomar 6 | |
|---|---|
|
| |
| Observation data ( J2000 epoch) | |
| Class | XI |
| Constellation | Ophiuchus |
| Right ascension | 17h 43m 42.20s [1] |
| Declination | −26° 13′ 21.0″ [1] |
| Distance | 25.02 ± 0.62 kly (7.67 ± 0.19 kpc) [2] |
| Physical characteristics | |
| Mass | 2.28×105 [3] M☉ |
| Metallicity | = –0.91 [3] dex |
| Estimated age | 12.4 ± 0.9 Gyr [2] |
| Other designations | ESO 520-21, GCl 75, 1740-262 [1] |
Palomar 6 is a loose globular cluster in the constellation Ophiuchus that belongs to the Milky Way galaxy. It is a member of the Palomar Globular Clusters group. It is located about 25,000 light-years (7,700 parsecs) away from the Sun. [2] It formed in what would become the bulge of the Milky Way. It is similar to other old-bulge globular clusters such as Messier 62, NGC 6522, NGC 6558, and Haute-Provence 1. [2]
First discovered on the National Geographic Society – Palomar Observatory Sky Survey plates by Robert G. Harrington and Fritz Zwicky, [4] it was catalogued as a globular cluster, and is one of four globulars known to contain a planetary nebula.
References
- ^ a b c "SIMBAD Astronomical Database". Results for Palomar 6. Retrieved 2009-10-04.
- ^ a b c d Souza, S. O.; Valentini, M.; Barbuy, B.; Pérez-Villegas, A.; Chiappini, C.; Ortolani, S.; Nardiello, D.; Dias, B.; Anders, F.; Bica, E. (2021). "Photo-chemo-dynamical analysis and the origin of the bulge globular cluster Palomar 6". Astronomy & Astrophysics. 656: A78. arXiv: 2109.04483. doi: 10.1051/0004-6361/202141768. S2CID 237485386.
- ^ a b Boyles, J.; et al. (November 2011), "Young Radio Pulsars in Galactic Globular Clusters", The Astrophysical Journal, 742 (1): 51, arXiv: 1108.4402, Bibcode: 2011ApJ...742...51B, doi: 10.1088/0004-637X/742/1/51, S2CID 118649860.
- ^ Abell, George O. (1955). "Globular Clusters and Planetary Nebulae Discovered on the National Geographic Society-Palomar Observatory Sky Survey". Publications of the Astronomical Society of the Pacific. 67 (397): 258. Bibcode: 1955PASP...67..258A. doi: 10.1086/126815.
External links
-
Media related to
Palomar 6 at Wikimedia Commons
- Simbad reference data
- SEDS: Palomar 6, Capricornus Dwarf
- Palomar 6 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- NASA Astronomy Picture of the Day: Palomar 6: Globular Star Cluster (19 October 2021)
|
| This star cluster–related article is a stub. You can help Wikipedia by expanding it. |