Investigation of the Be star phenomenon using the DENIS data

Details Investigation of the Be star phenomenon using the DENIS data Investigation of the Be star phenomenon using the DENIS data

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.217..225b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 217, no. 1-2, p. 225-226

Astronomy and Astrophysics

Astronomy

B Stars, Infrared Astronomy, Interstellar Magnetic Fields, Interstellar Matter, Near Infrared Radiation, Sky Surveys (Astronomy), Stellar Color, Stellar Mass Ejection, Stellar Spectra, Astronomical Photometry, Correlation, Detection, Diagrams, Stellar Physics

Scientific paper

Taking advantage of the fact that Be stars produce a characteristic infrared excess, the Deep Near-Infrared Survey (DENIS) data -- in combination with UBV and Infrared Astronomy Satellite (IRAS) photometric data -- can provide us with a quite complete sample of Be stars within about 4 kpc around the sun. This will give us the possibility to carry out further studies to see if their presence is correlated with particular physical characteristics of the interstellar medium surrounding them.

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