2 papers
astro-ph2008
Determinationm of Effective Temperatures and Luminosities of Rotating Stars
A. Gillich, R. Deupree, C. Lovekin +2
Spectral energy distributions for models of arbitrarily rotating stars are computed using two dimensional rotating stellar models, NLTE plane parallel model atmospheres, and a code…
astro-ph2007
Why are some A stars magnetic, while most are not?
G. A. Wade, J. Silvester, K. Bale +21
A small fraction of intermediate-mass main sequence (A and B type) stars have strong, organised magnetic fields. The large majority of such stars, however, show no evidence for mag…