Publication Date:
2013-08-31
Description:
The 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.
Keywords:
ASTROPHYSICS
Type:
NASA, Ames Research Center, Interstellar Dust: Contributed Papers; p 197-198
Format:
application/pdf
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