J
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Last name: JANKOV
First name: S.
n/a, MmSAI 77, p. 429 (2006)
International audience
International audience
International Workshop Active OB-Stars: Laboratories for Stellar & Circumstellar Physics, n/a, (2006)
Active OB stars : laboratories for stellar and circumstallar physics, Hokkai-Gakuen University, n/a, (2005)
International Workshop Active OB-Stars: Laboratories for Stellar & Circumstellar Physics, n/a, (2006)
New Interferometric Constraints on the Physics of Active OB-Stars, eds. S. Stefl, S. P. Owocki and A. T. Okazaki, 351, p. 57 (2007)
International audience
Astron. & Astrophys., 453, p. 1041 (2006)
ESO Workshop: Recent Scientific Results and 2nd Generation VLTI Instrumentation, n/a, (2006)
n/a, pages (2006)
Astron. and Astroph., 418, pp. 781-794 (2004)
n/a, pages (2006)
Astronomy and Astrophysics, v. 448, p. 1225-1234, 2006. http://dx.doi.org/10.1051/0004-6361:20052806
Astron. & Astrophys., 442, p. 567 (2005)
VizieR On-line Data Catalog: J/A+A, 409, p. 275 (2003)
Astron. & Astrophys., 448, pp. 1225-1234 (2006)
Astronomy and Astrophysics, v. 448, p. 1225-1234, 2006. http://dx.doi.org/10.1051/0004-6361:20052806
Astron. and Astroph., 407, pp. L47-L50 (2003)
Astron. & Astrophys., 409, pp. 275-286 (2003)
Conference on Scientific highlights 2003, eds. Combes and D. Barret, SF2A 217, (2003)
Astron. & Astrophys., 422, pp. 193-203 (2004)
Context. As previously demonstrated on Achernar, one can derive the angular radius, rotational velocity, axis tilt, and orientation of a fast-rotating star from the differential phases obtained by spectrally resolved long baseline interferometry using earth-rotation synthesis. Aims: We applied this method on a small sample of stars for...
Astron. & Astrophys., 411, p. 565 (2003)
Astron. & Astrophys., 411, p. 565 (2003)