Vulpecula OB1 is an OB association in which a batch of massive stars are being born. It was first identified by W. W. Morgan et al. (1953).[4] The association is located in the Orion Arm about 7,500[5] light-years away from the Sun. Nebulae that are contained in this association include NGC 6820 and NGC 6823,[4] plus Sharpless 2-88.[5]
| Vulpecula OB1 | |
|---|---|
Vulpecula OB1 | |
| Observation data (J2000 epoch) | |
| Constellation | Vulpecula |
| Right ascension | 19h 44.0m [1] |
| Declination | +24° 13′[1] |
| Mean distance | 5.2 kly (1.6 kpc)[2] |
| Radial velocity | 3.1[3] km/s |
| Physical characteristics | |
| Other designations | Vul OB1[1] |
| See also: Stellar association, Moving groups | |