IRDC 19175-4 and IRDC 19175-5 turbulence maps (Beuther+, 2009)

Physics

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Molecular Clouds, Millimetric/Submm Sources, Radio Lines

Scientific paper

The aims is to characterizing the gas and dust properties prior to and in the neighborhood of active intermediate- to high-mass star formation.
Two Infrared Dark Clouds (IRDCs), IRDC 19175-4 and IRDC 19175-5, that are located in the vicinity of the luminous massive star-forming region IRAS 19175+1357, but that remain absorption features up to 70um wavelength, were observed with the Plateau de Bure Interferometer in the 3.23mm dust continuum as well as the N2H+(1-0) and 13CS(2-1) line emission.
(2 data files).

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