Volume 387, Number 3, June I 2002
|Page(s)||1003 - 1012|
|Section||Interstellar and circumstellar matter|
|Published online||17 May 2002|
Circumstellar disks around Herbig Ae/Be stars: Polarization, outflows and binary orbits
Indian Institute of Astrophysics, Bangalore 560 034, India
Corresponding author: G. Maheswar, email@example.com
Accepted: 25 March 2002
The geometrical relationship between the distribution of circumstellar matter, observed optical linear polarization, outflows and binary orbital plane in Herbig Ae/Be stars is investigated. Optical linear polarization measurements carried out for a number of Herbig Ae/Be stars that are either known to be in binary systems and/or have bipolar jets are presented in this paper. Available information on the position angles of polarization, outflows and binary companions for Herbig Ae/Be stars is compiled and analysed for any possible correlations. In ≈ of the sources the outflow position angle is within of being parallel or perpendicular to the polarization position angle. In ≈ of the sources the binary position angle is within of being parallel or perpendicular to the polarization position angle. Out of 15 sources with bipolar outflows, 10 sources have the binary position angle within of being perpendicular to the outflow position angle. These results favour those binary formation mechanisms in which the binary components and the disks around individual stars or circumbinary disks are coplanar.
Key words: stars: pre-main sequence / stars: binaries: general / stars: circumstellar matter / ISM: jets and outflows / polarization / scattering
© ESO, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.