Photometric determination of spectral types for Be stars - The Q method

Details Photometric determination of spectral types for Be stars - The Q method Photometric determination of spectral types for Be stars - The Q method

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..465h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 687, p. 465-467.

Astronomy and Astrophysics

Astronomy

11

Astronomical Photometry, B Stars, Emission Spectra, Stellar Models, Astronomical Spectroscopy, Main Sequence Stars, Stellar Evolution, Stellar Spectra, Ubv Spectra

Scientific paper

The Q method of photometric spectral classification, which is useful as
a 'quick look' procedure by means of which to derive the spectral types
of normal B stars, is here shown to be equally useful for Be and Be
shell stars with only minor modifications. Attention is given to the
case where only photometric data are available for faint Be stars.

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