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Hydrogen Cyanide in the Bipolar Source CEP A

Published online by Cambridge University Press:  04 August 2017

L. Weliachew ,
D. T. Emerson ,
T. Forveille ,
J. H. Bieging ,
M.C.H. Wright  and
J. Ellder
L. Weliachew
Affiliation:
IRAM, Voie 10, Domaine Universitaire, 38406 St. Martin d'Hères Cédex, FRANCE
D. T. Emerson
Affiliation:
IRAM, Voie 10, Domaine Universitaire, 38406 St. Martin d'Hères Cédex, FRANCE
T. Forveille
Affiliation:
Group d'Astrophysique, CERMO, B.P. 68, 38402 St. Martin d'Hères Cédex, France
J. H. Bieging
Affiliation:
Radio Astronomy Laboratory, University of California, Berkeley, CA 94720 USA
M.C.H. Wright
Affiliation:
Radio Astronomy Laboratory, University of California, Berkeley, CA 94720 USA
J. Ellder
Affiliation:
Onsala Space Observatory, Chalmers University of Technology, S-439 00 Onsala, Sweden

Extract

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The Cep A molecular cloud has been mapped in the 87 GHz continuum and in the J = 1-0 transition of HCN with a combination of single antenna and interferometer observations. The resolution is 19″x14″ (about 0.06 pc at the distance of Cep A) and 0.8 km/sec in velocity.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 360
Copyright
Copyright © Reidel 1987