Are passive protostellar disks stable to self-shadowing?

Astronomy and Astrophysics

Volumn 361, Issue 1, 2000, Pages

  Dullemond, C P ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Accretion, accretion disks; Circumstellar matter; Infrared: stars; Stars: formation, pre main sequence

Indexed keywords

EID: 0001891078     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (3)

1. Adams, F. C., Lada, C. J., and Shu, F. H., 1987, ApJ 312, 788
2. Adams, F. C. and Shu, F. H., 1986, ApJ 308, 836
3. Bell, K. R., 1999, ApJ 526, 411