Hot, Warm, and Cold Cores: Goldilocks Meets Massive Star Formation

Details Hot, Warm, and Cold Cores: Goldilocks Meets Massive Star Formation Hot, Warm, and Cold Cores: Goldilocks Meets Massive Star Formation

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004jkas...37..265k&link_type=abstract

Journal of the Korean Astronomical Society, vol. 37, no. 4, pp. 265-268

Astronomy and Astrophysics

Astronomy

Stars: Formation, Ism: Clouds, (Ism:) Hii Regions, Ism: Molecules

Scientific paper

Molecular clouds present many levels of structure, including clumps and cores of varying size and density. We present a brief summary of these cores, describing their observed physical properties and their place in the star formation process. We conclude with some speculation about pre-proto-stellar stages of molecular cores and the observational challenges in their observation.

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