Thirteen-color photometry of Be stars

Details Thirteen-color photometry of Be stars Thirteen-color photometry of Be stars

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981rmxaa...6..163a&link_type=abstract

(International Astronomical Union, Reunion Regional Latinoamericana de Astronomia, 2nd, Merida, Venezuela, Jan. 19-23, 1981) Rev

Astronomy and Astrophysics

Astronomy

22

B Stars, Stellar Color, Stellar Magnitude, Stellar Spectrophotometry, Variable Stars, Color-Color Diagram, Giant Stars, Infrared Spectra, Interstellar Extinction, Periodic Variations, Shell Stars, Spectral Energy Distribution, Stellar Envelopes, Stellar Temperature, Supergiant Stars, Ultraviolet Spectra

Scientific paper

Thirteen-color photometry made at the San Pedro Matir Observatory in Baja California for a number of spectroscopically variable Be and shell stars is presented. Several of these stars show photometric variability in the UV and/or IR over a time base of two to three years. The more interesting stars are analyzed in terms of color-color diagrams, color excesses, spectral characteristics and changes in their energy distributions. Prospects for future research are discussed.

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