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A Study of Continuum Emission at 3.5 mm from Selected H II Regions

Published online by Cambridge University Press:  04 August 2017

M. A. Gordon ,
P. R. Jewell ,
M.A. Kaftan-Kassim  and
C. J. Salter
M. A. Gordon
Affiliation:
National Radio Astronomy Observatory Tucson, AZ 85721-0655 USA
P. R. Jewell
Affiliation:
National Radio Astronomy Observatory Tucson, AZ 85721-0655 USA
M.A. Kaftan-Kassim
Affiliation:
National Radio Astronomy Observatory Tucson, AZ 85721-0655 USA
C. J. Salter
Affiliation:
National Radio Astronomy Observatory Tucson, AZ 85721-0655 USA

Extract

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As the first part of a program to investigate the thermal emission of dust at millimeter wavelengths, we present maps of the continuum emission from radio-bright HII regions. These maps have been made with a filled aperture telescope, the NRAO 12-m telescope at Kitt Peak, with a HPBW of 70 arc seconds at 3.5 mm. We used a switched dual-beam technique and a restoration algorithm developed by Emerson et al. (1979 Astron. Ap. 76, 92). We compare these maps with maps made at centimeter wavelengths.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 190 - 191
Copyright
Copyright © Reidel 1987