Astron. & Astrophys., 453, pp. 1059-1066 (2006)
Astron. & Astrophys., 474, pp. L49-L52 (2007)
Astron. and Astroph., 410, pp. 375-388 (2003)
We present a prospective work undertaken on Spectro-Polarimetric INterferometry (SPIN). Our theoretical studies suggest that SPIN is a powerful tool for studying the mass loss from early type stars where strong Thomson scattering is present. Based on Monte Carlo simulations, we computed the expected SPIN signal for numerous hot star spectral...
International audience
Using 2D models of rotating stars, the interferometric measurements of alpha Eri and its fundamental parameters corrected for gravitational darkening effects we infer that the star might have a core rotating 2.7 times faster than the surface. We explore the consequences on spectral lines produced by surface differential rotation combined with...
Using 2D models of rotating stars, the interferometric measurements of alpha Eri and its fundamental parameters corrected for gravitational darkening effects we infer that the star might have a core rotating 2.7 times faster than the surface. We explore the consequences on spectral lines produced by surface differential rotation combined with...
International audience
Active OB-Stars: Laboratories for Stellare and Circumstellar Physics, eds. S. Stefl, S. Owocki and A. Okazaki, ASP Conference Series 361, p. 542 (2007)
Astron. and Astroph., 400, pp. 385-392 (2003). http://dx.doi.org/10.1051/0004-6361:20021834
International audience
SF2A-2007: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, eds. J. Bouvier, A. Chalabaev and C. Charbonnel, n/a, p. 489 (2007)