Hostname: page-component-cb9f654ff-k7rjm Total loading time: 0 Render date: 2025-09-01T17:13:28.880Z Has data issue: false hasContentIssue false
  • English
  • Français

A Nitrogen Rich OB Supergiant in the Large Magellanic Cloud

Published online by Cambridge University Press:  25 April 2016

A.R. Hyland  and
M.S. Bessell
A.R. Hyland
Affiliation:
Mount Stromlo and Siding Spring Observatory, Research School of Physical Sciences, Australian National University
M.S. Bessell
Affiliation:
Mount Stromlo and Siding Spring Observatory, Research School of Physical Sciences, Australian National University
Get access Rights & Permissions [Opens in a new window]

Extract

Recent spectroscopic investigations of OB stars by Walborn (1970,1971a) have revealed the existence of OB stars with anomalous nitrogen and carbon spectra. In particular, two groups of stars were identified — those with strong nitrogen features and accompanying weak carbon-oxygen blends (called ON stars), and those with weak nitrogen features and strong carbon features (called OC stars). These groups bear a striking resemblance to the WN, WC dichotomy exhibited by the Wolf Rayet stars and is suggestive that a common process may be responsible for both phenomena.

Information

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 6 , October 1975 , pp. 353 - 355
Copyright
Copyright © Astronomical Society of Australia 1975

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Article purchase

Temporarily unavailable

References

Ardeberg, A., Brunet, J.-P., Maurice, E., and Prévot, L., Astron. Astrophys. Suppl. 6, 249 (1972)Google Scholar
Brucato, R.J., and Mihalas, D., Mon. Not. R. Astron. Soc, 154, 491 (1971).CrossRefGoogle Scholar
Conti, P.S., Astrophys. J., 179, 161 (1973).CrossRefGoogle Scholar
Feast, M.W., Thackeray, A.D., and Wesselink, A.J., Mon. Not. R. Astron. Soc, 121, 337 (1960).CrossRefGoogle Scholar
Fehrenbach, C., and Duflot, M., Astron. Astrophys. Special Suppl. Ser. 1 (1970).Google Scholar
Lester, J.B., Astrophys. J., 185, 253 (1973).CrossRefGoogle Scholar
Mihalas, D., Hummer, D.G., and Conti, P.S., Astrophys. J. (Lett.), 175, L99 (1972).CrossRefGoogle Scholar
Walborn, N.R., Astrophys. J. (Lett.), 161, L149 (1970).CrossRefGoogle Scholar
Walborn, N.R., Astrophys. J. (Lett.), 164, L67 (1971a).CrossRefGoogle Scholar
Walborn, N.R., Astrophys. J. Suppl., 23, 257 (1971b).CrossRefGoogle Scholar
Walborn, N.R., Astron. J., 77, 312 (1972a).CrossRefGoogle Scholar
Walborn, N.R., Astrophys. J. (Lett.), 176, L119 (1972b).CrossRefGoogle Scholar