Growth of the line-profile variation region during Be episodes in lambda Eridani

Details Growth of the line-profile variation region during Be episodes in lambda Eridani Growth of the line-profile variation region during Be episodes in lambda Eridani

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.221..459k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 221, no. 1-2, p. 459-461

Physics

B Stars, Emission Spectra, Stellar Mass, Stellar Physics, Stellar Rotation, Variability, Angular Momentum, Line Spectra, Mass Distribution, Photosphere

Scientific paper

We have found that the range in wavelength of the line-profile
variations (lpv) in the Be star lambda Eridani increases by some 20%
during its emission phases. This growth is associated with a possible
increase in the equatorial velocity of the star during emission.

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