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Bright Young Star Candidates in the Rosette Nebula

Published online by Cambridge University Press:  12 April 2016

P.S. Chiang ,
W.P. Chen ,
J.Z. Li  and
Y.-H. Chu
P.S. Chiang
Affiliation:
Graduate Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
W.P. Chen
Affiliation:
Graduate Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
J.Z. Li
Affiliation:
Graduate Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
Y.-H. Chu
Affiliation:
Department of Astronomy, University of Illinois, Urbana-Champaign, IL, 61801, USA

Abstract

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We identified possible optical young stars in the Rosette Nebula by using the IRAS and the ROSAT databases. The previously reported “diffuse” X-ray emission has been resolved into point sources. Forty-seven point sources are detected above 3-sigma of the X-ray background, and twenty-seven of these have stellar counterparts. Some of the young star candidates appear to be associated Herbig-Haro nebular features.

Type
VII. Science With Small Telescopes
Information
International Astronomical Union Colloquium , Volume 183: Small-Telescope Astronomy on Global Scales , 2001 , pp. 335 - 336
Copyright
Copyright © Astronomical Society of the Pacific 2001

References

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