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Multiband far-infrared observations of the NGC 6334 complex

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/164112· OSTI ID:5496808
Multiband far-infrared (20-155 microns) observations of the large H II region/molecular cloud complex NGC 6334 are presented. The observations were performed simultaneously in four bands with effective wavelengths 21, 42, 71, and 134 microns. Eight far-infrared sources were detected which cover the range from sources with little of no continuum radio emission to well-developed H II regions. Maps of dust temperature and far-infrared optical depth of the complex are presented which reveal large-scale variations in the color temperature and optical depth. Star formation in the complex is discussed and it is concluded that a Rayleigh-Taylor instability generated by the gravitational attraction of the galactic plane can explain the regular separation of the far-IR sources. 40 references
Research Organization:
Univ. College, Dublin, Ireland; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
OSTI ID:
5496808
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 303; ISSN ASJOA
Country of Publication:
United States
Language:
English

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