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The B[e] Star MWC 84 (CI Cam)

Published online by Cambridge University Press:  12 April 2016

Carlos Jaschek  and
Yvette Andrillat
Carlos Jaschek
Affiliation:
Observatoire de Strasbourg, URA 1280 (CNRS), 11 rue de, l’Université, F-67000 Strasbourg, France- (deceased)
Yvette Andrillat
Affiliation:
Laboratoire d’Astronomie (072), URA 1280 (CNRS), Université de Montpellier II, Place Eugène Bataillon, F-34095 Montpellier Cédex 05, France

Extract

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The star MWC 84 (CI Cam) was first discovered to be an emission line object classified Bep (Merrill & Burwell, 1933), then classified as a symbiotic star and finally identified as the possible optical counterpart of the X-ray transient XTE J0421+560 (Wagner & Starrfield, 1998)

We have observed MWC 84 at the Haute Provence Observatory (CNRS) with a resolution of about 1.3 Å in 1992 (wavelength regions Hα and near infrared), 1998 and 1999 (from 4080 to 8880 Å).

Type
1. Overview
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 83 - 86
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Garcia, M.R., Berlind, P., Barton, E., McClintock, J.E., Calanan, P.J. McCarthy, J. 1998, IAUC 6865 Google Scholar
Hjellming, R.M., Mioduszewski, A.J. 1998a, IAUC 6857 Google Scholar
Hjellming, R.M., Mioduszewski, A.J. 1998b, IAUC 6862 Google Scholar
Hjellming, R.M., Mioduszewski, A.J. 1998b, IAUC 6872 Google Scholar
Merril, P.W., Burwell, C.G. 1933, ApJ 78, 86 Google Scholar
Wagner, R.M., Starrfield, S.G. 1998, IAUC 6857 Google Scholar