Pulsationally-Induced Changes in BW Vul's Photosphere

Details Pulsationally-Induced Changes in BW Vul's Photosphere Pulsationally-Induced Changes in BW Vul's Photosphere

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..494s&link_type=abstract

Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere

Physics

Scientific paper

Multiwavelength spectral syntheses suggest that BW Vul's atmospheric
T(τ) is generally steepened due to the pulsations. Line weakening
during shock phases is probably caused by a markedly decreased
temperature gradient.

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