Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-30T12:34:47.723Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectea of Of and Be Stabs in the near Infrared Region up to 1.1μ

Published online by Cambridge University Press:  12 April 2016

Yvette Andrillat
Yvette Andrillat*
Affiliation:
Observatoire de Haute Provence

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.

The classification of Of stars presents a number of problems, in part due to the small interval of the spectrum explored up to now. With J.M. Vreux an extended study has been made in the infrared region, up to 1.1μ. Be stars have been studied with L. Houziaux, The hydrogen Paschen lines and lines of helium I and II can be studied in the region and used to determine temperature class and luminosity.

Type
III Criteria and Applications Outside the MK Domain
Information
International Astronomical Union Colloquium , Volume 47: Spectral Classification of the Future , 1979 , pp. 137 - 150
Copyright
Copyright © Vatican Observatory 1979

References

Abell, C. (1975). Bull. Am. Astron. Soc. 7, 296.Google Scholar
Andrillat, Y., Baranne, A. and Duchesne, M. (1973). Mem. Soc. Roy. Liege V, 51.Google Scholar
Andrillat, Y. and Houziaux, L. (1967). Publ. OHP 8 n°11.Google Scholar
Andrillat, Y. and Houziaux, L. (1967a). Publ. OHP 9 n°32 = 1967, Journal des Observateurs 50, fasc. 4.Google Scholar
Andrillat, Y. and Houziaux, L. (1968). Publ. OHP 10 n°1 = 1968, Journal des Observateurs 51, fasc. 3.Google Scholar
Andrillat, Y. and Houziaux, L. (1972). Astrophys. Space Science 18, 324.Google Scholar
Andrillat, Y. and Vreux, J.M. (1974). de, Acad. R. Belgique - Bull, classe des Sciences LX 53 série, 430.Google Scholar
Andrillat, Y. and Vreux, J.M. (1975). Astron. Astrophys. 41, 133.Google Scholar
Andrillat, Y. and Vreux, J.M. (1978). submitted for publication in Astron. Astrophys. in pressGoogle Scholar
Auer, L.J. and Mihalas, D. (1972). Astrophys. J. Suppl. 24, 193.CrossRefGoogle Scholar
Conti, P.S. (1974). Astrophys. J. 187, 539.Google Scholar
Houziaux, L. and Andrillat, Y., (1976). In IAU Symp. No. 70. Be and Shell Stars, Slettebak, A., ed., D Reidel, Dordrecht, p. 87.CrossRefGoogle Scholar
Klein, R.I. and Castor, J.I. (1978). Astrophys. J. 220, 902.CrossRefGoogle Scholar
Mihalas, D. and Lockwood, G.W. (1972). Astrophys. J. 175, 757.Google Scholar
Nussbaumer, H. (1971). Astrophys. J. 170, 93.Google Scholar
Vreux, J.M. and Andrillat, Y. (1975-6). Acad. R. Belgique - Bull, classe des Sciences. LXI 5e série, 577.CrossRefGoogle Scholar
Vreux, J.M. and Andrillat, Y. (1978). submitted for publication in Astron. Astrophys. in pressGoogle Scholar
Walborn, N.R. (1972). Astron. J. 77, 312.CrossRefGoogle Scholar
Walborn, N.R. (1973). Astron. J. 78, 1067.Google Scholar