Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-17T23:16:25.635Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Feigelson, E.D. & Montmerle, T. 1999, ARA&A, 37, 363 Google Scholar
Cox, P., Deharveng, L., & Leene, A. 1990, A&A, 230,181 Google Scholar
Pérez, M.R., 1991, RMxAA, 22, 99 Google Scholar