Abstract
An important factor is the relation of HAEBE stars with other groups of peculiar early type stars, such as Be and B[e] stars, luminous blue variables (LBVs) etc. In many cases Polarimetric properties of HAEBE stars and B[e] (Be) stars are similar. We have carried out a Polarimetric study of peculiar early-type stars with the following aims:
-
1.
First, to obtain new Polarimetrie (linear and circular) data for a large group of HAEBE stars and candidate members, as well as for some peculiar Be and B[e] stars and LBVs. The whole list of programme stars consists of 60 objects located mainly in the southern hemisphere. For 40 of the 60 objects Polarimetrie data have been obtained for the first time.
-
2.
Second, to study Polarimetrie variability of the programme stars on different time-scales (minutes ... hours ...days).
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsAuthor information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1998 Springer Science+Business Media Dordrecht
About this chapter
Cite this chapter
Yudin, R.V., Evans, A. (1998). Polarimetry of Southern Peculiar Early-Type Stars. In: Hubert, A.M., Jaschek, C. (eds) B[e] Stars. Astrophysics and Space Science Library, vol 233. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9014-3_20
Download citation
DOI: https://doi.org/10.1007/978-94-015-9014-3_20
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5080-9
Online ISBN: 978-94-015-9014-3
eBook Packages: Springer Book Archive