Published in

Cambridge University Press, Proceedings of the International Astronomical Union, H15(5), p. 403-403, 2009

DOI: 10.1017/s1743921310009932

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Atomic carbon in an infrared dark cloud

Journal article published in 2009 by Volker Ossenkopf ORCID, Chris W. Ormel, Robert Simon, Kefeng Sun, Jürgen Stutzki
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

Infrared dark clouds (IRDCs) are potential sites of massive star formation, dark in the near-infrared, but in many cases already with indications of active star-formation from far-infrared and submm observations. They are an ideal test bed to study the role of internal and external heating on the structure of the molecular cloud material.