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2012MNRAS.422.3178E - Mon. Not. R. Astron. Soc., 422, 3178-3188 (2012/June-1)
Star formation towards the Scutum tangent region and the effects of galactic environment.
EDEN D.J., MOORE T.J.T., PLUME R. and MORGAN L.K.
Abstract (from CDS):
Despite having a very high star formation rate, and containing at least one cloud with a very high CFE, the star formation associated with the Scutum-Centaurus tangent does not appear to be in any way abnormal or different to that in the other two spiral arm sections. Large variations in the CFE are found on the scale of individual clouds, however, which may be due to local triggering agents as opposed to the large-scale Galactic structure.
Abstract Copyright: 2012 The Author Monthly Notices of the Royal Astronomical Society2012 RAS
Journal keyword(s): stars: formation - ISM: clouds - ISM: individual objects: W43 - Galaxy: kinematics and dynamics
VizieR on-line data: <Available at CDS (J/MNRAS/422/3178): table1.dat table2.dat table3.dat>
Simbad objects: 927
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