In:
International Astronomical Union Colloquium, Cambridge University Press (CUP), Vol. 120 ( 1989), p. 424-431
Abstract:
The Draco nebula, the faint reflection nebulosity LBN 406/412/415 (Lynds 1965) at 1≈91°, b≈38°, z≥500 pc (Goerigk and Mebold, 1986), contains delicate filaments at its low-1, low-b (SW) boundary (Goerigk et al. 1983, Mebold et al. 1985). The density in the boundary is characterized by the presence of molecules like CO and H 2 CO (Mebold et al. 1985) and NH 3 (Mebold et al. 1987). Johnson (1986) found an excess of unidentified IRAS point sources in the area of the Draco nebula, a large fraction of which is located close to the SW boundary.
Type of Medium:
Online Resource
ISSN:
0252-9211
DOI:
10.1017/S0252921100024192
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
1989
