Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-17T15:14:36.111Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectroscopic Observations of Be Stars Especially in the Infrared

Published online by Cambridge University Press:  14 August 2015

L. Houziaux  and
Y. Andrillat
L. Houziaux
Affiliation:
Institut d'Astrophysique, Université de Liège, Avenue de Cointe, 5, B-4200 Liège (Belgium)
Y. Andrillat
Affiliation:
Observatoire de Haute Provence, C.N.R.S., F-04870 St. Michel l'Observatoire, France

Extract

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.

Since the time of I.A.U. Colloquium n° 70, new data have been obtained in the infrared, far less however than in the ultraviolet or in the visible. Few line spectra have been recorded but numerous results have been published in the field of spectrometry of the continuum. It is however neither easy nor very useful to report on the infrared wavelength range alone, and therefore we shall consider when appropriate other spectral regions in this review. After all, the astrophysicist nowadays has the advantage to seek for information in a spectrum which encompasses a fantastic frequency range of about 10 dex, from ν = 108s−1 up to ν = 1018s−1. This means that a contemporary astronomer will have to become familiar with a somewhat larger span of phenomena than with the rather narrow one he has been accustomed to for the last 40 or 50 years.

Type
IV. Infrared Observations
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 211 - 228
Copyright
Copyright © Reidel 1982 

References

Altamore, A., Baratta, G.B., Casatella, A., Grasdalen, G.L., Persi, P. and Viotti, R.: 1980, Astron. and Astrophys., 90, p. 290.Google Scholar
Andrillat, Y. et Houziaux, L.: 1967, J. Observateurs, 50, p. 107.Google Scholar
Danks, A. and Houziaux, L.: 1978, Publ. Astron. Soc. Pac., 90, p. 453.Google Scholar
Delcroix, A.: 1979, private communication. Google Scholar
Garrison, M.L. Jr: 1978, Astrophys. J., 224, p. 535.Google Scholar
Johnson, H.L.: 1977, Rev. Mexicana Astron. y Astrofisica, 2, p. 71.Google Scholar
Kurucz, R.L., Peytremann, E. and Avrett, E.H.: 1974, Blanketed Model Atmospheres for Early-Type Stars, Smithsonian Institution.Google Scholar
Oegerle, W., Polidan, R. and Peters, G.: 1979, B.A.A.S., 11, p. 682 Google Scholar
Scargle, D.S., Erickson, E.F., Witteborn, F.C. and Strecker, D.W.: 1978, Astrophys. J., 224, p. 527 CrossRefGoogle Scholar
Smith, H.A., Thronson, H.A., Larson, H.P. and Fink, U.: 1979, B.A.A.S., 11, p. 668 Google Scholar
Thompson, G.I., Nandy, K., Jamar, C., Monfils, A. Houziaux, L., Carnochan, D.J. and Wilson, R.: 1978, Catalogue of Ultraviolet Stellar Fluxes, The Science Research Council, London.Google Scholar
Whittet, D.C.B., van Breda, I.G.: 1980, Monthly Notices R. Astron. Soc., 192, 467 Google Scholar