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 |