The Mopra DQS survey of the G333 region

M. R. Cunningham; I. Bains; N. Lo; T. Wong; M. G. Burton; P. A. Jones

doi:10.1017/S1743921307001925

The Mopra DQS survey of the G333 region

M. R. Cunningham, I. Bains, N. Lo, T. Wong, M. G. Burton, P. A. Jones

Research output: Contribution to journal › Article › peer-review

Abstract

Any successful model of star formation must be able to explain the low star forming efficiency of molecular clouds in our Galaxy. If the collapse of gas is regulated only by gravity, then the star formation rate should be orders of magnitude larger than the 1 M per year within our galaxy. The standard model invokes magnetic fields to slow down the rate of collapse, but does not explain star formation in cluster mode, or the lack of observed variations in the chemistry of molecular clouds if they are long-lived entities.

Original language	English (US)
Pages (from-to)	404
Number of pages	1
Journal	Proceedings of the International Astronomical Union
Volume	2
Issue number	S237
DOIs	https://doi.org/10.1017/S1743921307001925
State	Published - Aug 2006
Externally published	Yes

Keywords

ISM: clouds
ISM: molecules
Radio lines: ISM
Turbulence

ASJC Scopus subject areas

Medicine (miscellaneous)
Astronomy and Astrophysics
Nutrition and Dietetics
Public Health, Environmental and Occupational Health
Space and Planetary Science

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AU - Bains, I.

AU - Lo, N.

AU - Wong, T.

AU - Burton, M. G.

AU - Jones, P. A.

PY - 2006/8

Y1 - 2006/8

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AB - Any successful model of star formation must be able to explain the low star forming efficiency of molecular clouds in our Galaxy. If the collapse of gas is regulated only by gravity, then the star formation rate should be orders of magnitude larger than the 1 M per year within our galaxy. The standard model invokes magnetic fields to slow down the rate of collapse, but does not explain star formation in cluster mode, or the lack of observed variations in the chemistry of molecular clouds if they are long-lived entities.

KW - ISM: clouds

KW - ISM: molecules

KW - Radio lines: ISM

KW - Turbulence

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