Sutton, E. C. and Blake, Geoffrey A. and Masson, C. R. and Phillips, T. G. (1984) On the Interpretation of the broad-band millimeter-wave flux from Orion. Astrophysical Journal Letters, 283 (1). L41-L44. ISSN 2041-8205. http://resolver.caltech.edu/CaltechAUTHORS:20120911-115020538
- Published Version
See Usage Policy.
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20120911-115020538
Spectral observations of the core of Orion A at wavelengths around 1.3 mm show a high density of strong, broad emission lines. The combined flux in lines with peak antenna temperatures stronger than 0.2 K accounts for approximately 40 percent of the broad-band millimeter-wave flux from the region. Thus the broad-band flux from Orion A is in large part due to sources other than dust emission.
|Additional Information:||© 1984 American Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1984 April 3; accepted 1984 May 31. Single-dish millimeter-wave astronomy at the Owens Valley Radio Observatory is supported by NSF grant AST-8214693. The authors would like to thank R. E. Miller of AT & T Bell Laboratories, Murray Hill, for supplying the junctions used in this work. The authors are also grateful to D. P. Woody and S. L. Scott for their assistance and to Jocelyn Keene for helpful discussions.|
|Official Citation:||On the interpretation of the broad-band millimeter-wave flux from Orion Sutton, E. C.; Blake, G. A.; Masson, C. R.; Phillips, T. G.|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||11 Sep 2012 20:18|
|Last Modified:||29 Aug 2014 14:47|
Repository Staff Only: item control page