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A Photometric Study of Herbig Ae/Be Stars

Published online by Cambridge University Press:  23 September 2016

Eugenio E.  and
Mendoza V.
Eugenio E.
Affiliation:
Instituto de Astronomia, UNAM, P.O. Box 20-158, Mexico 20, D.F., 01000, Mexico
Mendoza V.
Affiliation:
Instituto de Astronomia, UNAM, P.O. Box 20-158, Mexico 20, D.F., 01000, Mexico

Extract

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It is well known (cf. Mendoza 1983) that “classical“ Be stars, and Herbig Ae/Be objects, in addition to hydrogen lines in emission, also share at least two photometric characteristics, namely, light varitions, and infrared color excesses.

We have selected the α(16)⋀(9) {Mendoza 1979}, and the JHKL-photometric systems, in order to study some photometric properties of Be stars. The observations have been carried out at the National Astronomical Observatory (San Pedro Martir, B.C.N., and Tonantzintla, Pue.), Mexico, from 1976 to 1986.

Type
V. Evolutionary Status of Be Stars
Information
International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 529 - 531
Copyright
Copyright © Cambridge University Press 1987

References

Mendoza, E.E., 1979 Astron. Astrophys. 71, 147.Google Scholar
Mendoza, E.E., 1983 Rev. Mexicana Astron. Astrof. 7, 141.Google Scholar