NGC 7510
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| NGC 7510 | |
|---|---|
 | |
| Observation data (J2000.0 epoch) | |
| Constellation | Cepheus |
| Right ascension | 23h 11.1m[1] |
| Declination | +60° 34′[1] |
| Distance | 11.4 kly (3.48 kpc)[2] |
| Apparent magnitude (V) | 7.9[1] |
| Apparent dimensions (V) | 7.0′[1] |
| Physical characteristics | |
| Estimated age | 107[3] |
NGC 7510 is an open cluster of stars located around 11,400[2] light years away in the constellation Cepheus, near the border with Cassiopeia.[3] At this distance, the light from the cluster has undergone extinction from interstellar gas and dust equal to E(B – V) = 0.90 ± 0.02 magnitude in the UBV photometric system.[2] Its brightest member is a giant star with a stellar classification of B1.5 III. This cluster forms part of the Perseus Spiral Arm.[4] It has a Trumpler class rating of II 2 m[2] and is around 10 million years old.[3]
References[edit]
- ↑ 1.0 1.1 1.2 1.3 James O'Meara, Stephen (2007), Steve O'Meara's Herschel 400 Observing Guide, Cambridge University Press, p. 278, ISBN 0521858933, https://books.google.com/books?id=Nyh9fAC_tpIC&pg=PA278.
- ↑ 2.0 2.1 2.2 2.3 Paunzen, E. et al. (November 2005), "CCD photometric search for peculiar stars in open clusters. VI. NGC 1502, NGC 3105, Stock 16, NGC 6268, NGC 7235 and NGC 7510", Astronomy and Astrophysics 443 (1): 157–162, arXiv:astro-ph/0508151, Bibcode 2005A&A...443..157P, doi:10.1051/0004-6361:20053287.
- ↑ 3.0 3.1 3.2 Barbon, R.; Hassan, S. M. (February 1996), "A new study of the young open cluster NGC 7510", Astronomy and Astrophysics Supplement 115: 325–332, Bibcode 1996A&AS..115..325B.
- ↑ Crossen, Craig; Rhemann, Gerald (2004), Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes, Springer, p. 78, ISBN 3211008519, https://books.google.com/books?id=mfJeWrJRqrkC&pg=PA78.
Joey (talk), Natalia (talk), 
ynoss (talk), or 
Daniel (older account/talk).
External links[edit]
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- NGC 7510 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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