Computer Science
Scientific paper
Nov 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..337..324v&link_type=abstract
The Nature and Evolution of Disks Around Hot Stars, ASP Conference Series, Vol. 337, Proceedings of a meeting held 7-9 July 2004
Computer Science
3
Scientific paper
The accepted driving mechanism for the mass loss in A-supergiants is radiation pressure. Several clues, however, point to a model of co-rotating clouds of gas and the existence of a weak magnetic field on the surface. We report on spectropolarimetric observations between 1999 and 2003 of 12 A-type supergiants taken with the MuSiCoS spectropolarimeter at the 2m Bernard Lyot telescope at the Pic-du-Midi. We present the values of the derived longitudinal component of the magnetic field. The significance of the results is discussed.
Geers Vincent Carlo
Gomez de Castro Ana Ines
Henrichs Hubertus F.
Schnerr R. S.
Talavera Antonio
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