Star formation in the giant molecular cloud

Details Star formation in the giant molecular cloud Star formation in the giant molecular cloud

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..154b&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 3, p. 154 - 158 (2005)

Astronomy and Astrophysics

Astronomy

Star Formation, Molecular Clouds

Scientific paper

Since most of the stars in the galaxy are considered to be formed in giant molecular clouds, studying star formation in those clouds is very important not only to recognize itself but also to investigate the galaxy formation and its evolution. We have carried out a deep near-infrared survey toward the C cloud of Vela Molecular Ridge which is located in southern hemisphere. In this article, I present a detailed study of an embedded cluster in this cloud as a preliminary result of the survey.

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