Abstract
We demonstrate the importance of Ha spectro-polarimetry in constraining the geometry of Herbig Ae/Be stars. We find that discs are common in Herbig Ae and Be stars, although different polarization signatures may imply different modes of accretion.
Original language | English |
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Title of host publication | In: Procs of the Hot Star Workshop III: the Earliest Stages of Massive Star Birth - ASP Conf Series Vol.267 |
Publisher | Astronomical Society of the Pacific |
Pages | 439-440 |
ISBN (Print) | 978-1-58381-603-5, 1-58381-107-9 |
Publication status | Published - 2002 |