R-associations III. Local optical spiral structure
Abstract
The galactic distribution of R-associations is investigated. They show that the local (Cygnus) spiral feature extends over 2 kpc in the direction of Vela (1 = 265 , and is clearly separated from the next inner (Carina-Sagittarius) spiral feature. There is some evidence for a concentration of the dust towards the inner edge of the local optical spiral feature, a phenomenon which is observed in external galaxies (Lynds 1970, 1972). The R-associations are combined with other good spiral tracers to produce a new map of optical spiral structure. A possible interpretation of this map is suggested in which the angle of inclination of the spiral arms is l3'i4%
- Publication:
-
The Astronomical Journal
- Pub Date:
- July 1975
- DOI:
- 10.1086/111771
- Bibcode:
- 1975AJ.....80..503H