Why do starless cores appear more flattened than protostellar cores?
Open Access
- 1 March 2002
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 330 (4) , 769-771
- https://doi.org/10.1046/j.1365-8711.2002.05166.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 7 references indexed in Scilit:
- Intrinsic Shapes of Molecular Cloud CoresThe Astrophysical Journal, 2001
- Dense Cores Mapped in Ammonia: A DatabaseThe Astrophysical Journal Supplement Series, 1999
- A survey for dense cores in dark cloudsThe Astrophysical Journal Supplement Series, 1989
- Candidate solar-type protostars in nearby molecular cloud coresThe Astrophysical Journal, 1986
- Testing for triaxiality with kinematic dataMonthly Notices of the Royal Astronomical Society, 1985
- Dense cores in dark clouds. II - NH3 observations and star formationThe Astrophysical Journal, 1983
- Dense cores in dark clouds. I - CO observations and column densities of high-extinction regionsThe Astrophysical Journal, 1983