Structure of the Dense Molecular Gas in the NGC 1333 IRAS 4 Region
- 20 December 2004
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 617 (2) , 1157-1166
- https://doi.org/10.1086/425898
Abstract
No abstract availableThis publication has 25 references indexed in Scilit:
- Modeling Line Profiles of Protostellar Collapse Observed with High Angular ResolutionThe Astrophysical Journal, 2002
- Infall, Outflow, Rotation, and Turbulent Motions of Dense Gas within NGC 1333 IRAS 4The Astrophysical Journal, 2001
- High‐Resolution Observations of the Molecular Clouds in the NGC 1333 IRAS 4 RegionThe Astrophysical Journal, 2001
- Physical Conditions in Regions of Star FormationAnnual Review of Astronomy and Astrophysics, 1999
- Berkeley‐Illinois‐Maryland Association Survey of Protostellar Collapse Candidates in HCO + and HCN LinesThe Astrophysical Journal Supplement Series, 1999
- New Protostellar Collapse Candidates: An HCO+Survey of the Class 0 SourcesThe Astrophysical Journal, 1997
- Modeling Line Profiles of Protostellar Collapse in B335 with the Monte Carlo MethodThe Astrophysical Journal, 1995
- A molecular line study of NGC 1333/IRAS 4The Astrophysical Journal, 1995
- From T Tauri stars to protostars: Circumstellar material and young stellar objects in the rho Ophiuchi cloudThe Astrophysical Journal, 1994
- Interstellar extinction in the vicinity of the reflection nebula NGC 1333 in PerseusAstrophysics and Space Science, 1990