Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004pabei..22..122q&link_type=abstract
Progress in Astronomy (ISSN 1000-8349), Vol. 22, No. 2, p. 122 - 133 (2004)
Astronomy and Astrophysics
Astrophysics
Astrophysics, Star Formation, Review, Collapse, Accretion Disk, Outflow, H Ii Regions
Scientific paper
It is well known that stars form in molecular clouds. Through almost 30 years' observation and study, astronomers come to a relatively clear agreement that low mass stars form by collapse, accretion and outflow. However, for massive star formation there still exist many indefinite factors. The observational results show that maybe massive stars form by collapse, accretion and outflow either, without excluding the possibility that massive stars form by coalescence. Low mass star forming regions include only low mass stellar objects, but massive star forming regions include not only massive stars but also low mass stars. Massive stars are associated with UCHII regions well in their embedded phase. This paper summarizes the results of observation and study for star formation in different phases. Massive star formation and star formation in star clusters will be very important in the future work.
Qin Sheng-Li
Wang Jun-Jie
Wu Yue-Fang
Zhao Gang
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