Maps of dust clouds at 1.3 millimeters associated with bright H II regions

Details Maps of dust clouds at 1.3 millimeters associated with bright H II regions Maps of dust clouds at 1.3 millimeters associated with bright H II regions

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...323..766g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 323, Dec. 15, 1987, p. 766-778.

Astronomy and Astrophysics

Astrophysics

24

Astronomical Photometry, Cosmic Dust, H Ii Regions, Molecular Clouds, Nebulae, Astronomical Maps, Emission Spectra, Far Infrared Radiation, Plasma Temperature

Scientific paper

Maps of the dust clouds associated with W3 Main, NGC 1976, NGC 2024, Sgr B2, M17, W49A, and W51A made at 1.3 mm show brightness distributions often very different from those seen in the FIR. These differences imply that the regions of maximum dust temperature generally do not correspond with regions of maximum column density. The authors give flux densities corrected for free-free emission.

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