How do dense cores embedded in a pc scale filamentary clouds form, by gas flow motions along filamentary clouds and/or contracting motions by themselves?

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천문학회보 (The Bulletin of The Korean Astronomical Society)

한국천문학회 (Korean Astronomical Society)

저자

Shinyoung Kim(Korea Astronomy and Space science Institute/University of Science and Technology)
Chang Won Lee(Korea Astronomy and Space science Institute/University of Science and Technology)
Philip C. Myers(Center for Astrophysics, Harvard-Smithsonian)
Paola Caselli(Max-Planck-Institut für Extraterrestrische Physik)
Mi-Ryang Kim(Korea Astronomy and Space science Institute)

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