Spectral classification of Be stars

Details Spectral classification of Be stars Spectral classification of Be stars

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.164..167h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 164, no. 1, Feb. 1990, p. 167-169.

Astronomy and Astrophysics

Astrophysics

3

B Stars, Stellar Spectra, Abundance, Hydrogen, Shell Stars, Stellar Rotation, Ubv Spectra

Scientific paper

The present work discusses the possibility of using the Q-value in spectral classification of Be stars. Also, it shows how the comparison between the spectral type obtained by the Q-method and any other method will help in detection of stars that are wrongly classified or those presenting discrepancy in spectral type due to peculiarity or rotation, by defining a new quantity Delta-Q.

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