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MON R2: A Blister Type H II Region

Published online by Cambridge University Press:  04 August 2017

M. Massi ,
M. Felli ,
M. Catarzi  and
M. Simon
M. Massi
Affiliation:
Osservatorio di Arcetri, Florence, Italy
M. Felli
Affiliation:
Osservatorio di Arcetri, Florence, Italy
M. Catarzi
Affiliation:
Osservatorio di Arcetri, Florence, Italy
M. Simon
Affiliation:
State University of New York, Stony Brook, N.Y. USA

Extract

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The compact H II region MONR2 has been studied with the VLA at 6 and 1.3 cm (Massi, Felli, and Simon 1985). With a resolution of 1″ the source is now well resolved. The H II region has a circular shape 27″ in diameter and a non uniform surface brightness distribution. The peak of the emission is concentrated in a small sharp strip along the SE edge.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 193
Copyright
Copyright © Reidel 1987 

References

Massi, M., Felli, M., and Simon, M.: 1985, Astron. Astrophys. in press.Google Scholar
Beckwith, S., Evans, N.J. II, Becklin, E.E., and Neugebauer, G.: 1976, Astrophys. J. 208, 390.CrossRefGoogle Scholar