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The Be/X-ray transient HD34921

Published online by Cambridge University Press:  12 May 2006

V. F. Polcaro ,
L. Norci ,
E. J. A. Meurs ,
S. Bernabei  and
A. S. Miroshnichenko
V. F. Polcaro
Affiliation:
IASF-INAF, Rome, Italy email: [email protected]
L. Norci
Affiliation:
School of Physics, Dublin City University, Dublin, Ireland
E. J. A. Meurs
Affiliation:
Dunsink Observatory, Dublin Institute for Advanced Studies, Castleknock, Dublin 15, Ireland
S. Bernabei
Affiliation:
Osservatorio Astronomico, Bologna, Italy
A. S. Miroshnichenko
Affiliation:
University of Toledo, USA
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Abstract

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HD34921 has been identified as the counterpart of the X-ray source 4U0515+38 (=1H0521+373). The InfraRed properties are reminiscent of the B[e] system CI Cam. Optical short-term variability suggests a compact companion. We discuss how this system fits in the overall framework of Be stars and X-ray binaries.

Keywords

Stars: B[e]Stars: X-raysStars: Neutron
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S230: Populations of High Energy Sources in Galaxies , August 2005 , pp. 49 - 50
Copyright
2006 International Astronomical Union