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Dust in a few southern H II regionsThe property of dust in four southern H II region/molecular cloud complexes (RCW 108, RCW 57, RCW 122, and G351.6-1.3) was discussed. These regions were observed at an effective wavelength of 150 micron using TIFR balloon borne 1 m telescope and deconvolved maps with a resolution of 1 min were obtained. The data were combined with other available data to derive the properties of the infrared emitting dust in these regions.
Document ID
19910005630
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ghosh, Swarna Kanti (Tata Inst. of Fundamental Research Bombay, India)
Iyengar, K. V. K. (Tata Inst. of Fundamental Research Bombay, India)
Rengarajan, T. N. (Tata Inst. of Fundamental Research Bombay, India)
Tandon, S. N. (Tata Inst. of Fundamental Research Bombay, India)
Verma, R. P. (Tata Inst. of Fundamental Research Bombay, India)
Daniel, R. R. (Tata Inst. of Fundamental Research Bombay, India)
Date Acquired
September 6, 2013
Publication Date
December 1, 1989
Publication Information
Publication: NASA, Ames Research Center, Interstellar Dust: Contributed Papers
Subject Category
Astrophysics
Accession Number
91N14943
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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