Density structure of globules at different evolutionary stages

Details Density structure of globules at different evolutionary stages Density structure of globules at different evolutionary stages

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..228k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 4, p. 228 - 233 (2005)

Astronomy and Astrophysics

Astronomy

Globules, Density Structure, Star Formation

Scientific paper

Stars are thought to be formed in dense molecular cloud cores. It, however, still remains unclear that how and when the star formation process takes place. On the basis of extinction (AV) measurements of both starless and star-forming globules (isolated dense cores) at the near-infrared wavelengths. I investigated their density structure using the Bonnor-Ebert sphere model. Here I present important findings on the density structure, stability, and evolution of globules.

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