Molecular line study of massive star forming regions from the RMS survey

Abstract

In this paper we selected a sample of massive star forming regions from the Red MSX Source (RMS) survey, to study star formation activities (mainly outflow and inflow signatures).

References in corpus (4)

• The RMS Survey: Radio observations of candidate massive YSOs in the southern hemisphere
• The RMS Survey: ${}^{13}$CO observations of candidate massive YSOs in the northern Galactic plane
• A multi-transition molecular line study of inward motions towards massive star-forming cores
• Molecular line profiles as diagnostics of protostellar collapse: modelling the `blue asymmetry' in inside-out infall

Cited by in corpus (7)

• A search for ionized jets towards massive young stellar objects
• Hundreds of new cluster candidates in the VISTA variables in the Via Lactea survey DR1
• Chemical evolution of Red MSX Sources in the southern sky
• Extended HNCO, SiO, and HC${}_3$N emission in 43 southern star-forming regions
• HNCO: A Molecule Traces Low-velocity Shock
• Effects of infall and outflow on massive star-forming regions
• Physical and chemical properties of Red MSX Sources in the southern sky: HII regions