Issue |
A&A
Volume 507, Number 1, November III 2009
|
|
---|---|---|
Page(s) | 369 - 376 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/200811104 | |
Published online | 08 September 2009 |
The relation between
CO J = 2–1 line width in molecular clouds and bolometric luminosity of associated IRAS sources*
1
Department of Astronomy, School of Physics, Peking University, Beijing 100871, PR China e-mail: kwang@cfa.harvard.edu; yfwu@bac.pku.edu.cn
2
Department of Atmospheric Sciences, School of Physics, Peking University, Beijing 100871, PR China
3
Institut für Anorganische Chemie, Universität Bonn, Römer St. 164, 53117 Bonn, Germany
4
I. Physikal. Institut, Universität zu Köln, Zülpicher St. 77, 50937 Köln, Germany
Received:
7
October
2008
Accepted:
21
July
2009
Aims. We search for evidence of a relation between properties of young stellar objects (YSOs) and their parent molecular clouds to understand the initial conditions of high-mass star formation.
Methods. A sample of 135 sources was selected from the InfraRed Astronomical
Satellite (IRAS) point source catalog, on the basis of
their red color to enhance the possibility of discovering young
sources. Using the Kölner Observatorium für SubMillimeter
Astronomie (KOSMA) 3-m telescope, a single-point survey in
13CO was carried out for the entire
sample, and 14 sources were mapped further. Archival mid-infrared
(MIR) data were compared with the 13CO emissions to identify
evolutionary stages of the sources. A 13CO observed sample was
assembled to investigate the correlation between 13CO line
width of the clouds and the luminosity of the associated YSOs.
Results. We identified 98 sources suitable for star formation analyses for
which relevant parameters were calculated. We detected 18 cores from
14 mapped sources, which were identified with eight pre-UC H ii
regions and one UC H ii region, two high-mass cores earlier
than pre-UC H ii phase, four possible star forming clusters,
and three sourceless cores. By compiling a large (360 sources)
13CO observed sample, a good correlation was found between the
13CO line width of the clouds and the bolometric luminosity of
the associated YSOs, which can be fitted as a power law,
lg(ΔV13/ km s-1) = (-0.023±0.044) + (0.135±0.012)lg. Results show
that luminous (>103
) YSOs tend to be associated with
both more massive and more turbulent (ΔV13 > 2 km s-1) molecular cloud structures.
Key words: stars: formation / ISM: clouds / ISM: molecules / ISM: kinematic and dynamics
© ESO, 2009
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