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Radio emission from young stellar objects in the Rho Ophiuchi cloud

Published online by Cambridge University Press:  04 August 2017

Ph. André ,
T. Montmerle ,
E.D. Feigelson  and
P. Stine
Ph. André
Affiliation:
Service d'Astrophysique, C.E.N. Saclay 91 191 Gif-sur-Yvette Cedex, France
T. Montmerle
Affiliation:
Service d'Astrophysique, C.E.N. Saclay 91 191 Gif-sur-Yvette Cedex, France
E.D. Feigelson
Affiliation:
Penn State University, University Park, PA 16802, USA
P. Stine
Affiliation:
Penn State University, University Park, PA 16802, USA

Extract

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Following an Einstein X-ray survey of the rho Oph molecular cloud, uncovering several dozen young stellar objects (YSO) (Montmerle et al. 1983), an extensive radio continuum VLA(C) survey was conducted in 1983 to look for counterparts to these sources at 1.4 and 5 GHz (André et al. 1986) To shed light on emission mechanisms, we performed follow-up VLA(A/B) observations of identified radio stars in March 1985 at 1.4, 5 and 15 GHz.

Type
Bipolar Flows, Jets and Protostars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 61 - 62
Copyright
Copyright © Reidel 1987 

References

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