Abstract
Hot subdwarf stars are objects which are very suitable for studies of the older parts of our Galaxy. They belong to the brighter objects in such populations, and due to their blue colour and unique atmospheric properties they are easily found and unambiguously identified.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Allen, C., & Santillan, A., 1991, RMxA, 22, 255
Altmann, M., 2002, PhD. Thesis, in prep.
Altmann, M., & de Boer, K.S. 2000, A&A, 353, 135
Altmann, M., de Boer, K.S., Edelmann, H. 2001, AN, 322, 397
Altmann, M., Edelmann, H., de Boer, K.S. 2002, A&A, to be submitted
de Boer, K.S., Aguilar Sanchez, Y., Altmann, M., & et al. 1997, A&A 327, 577
D’Cruz, N.L., Dorman, B., Rood, R.T., O’Connell, R.W., 1996, ApJ, 466, 359
Maxted, P.F.L., Heber, U., Marsh, T.R., North, R.C., 2001, MNRAS, 326, 1391
Ojha, D.K., Bienayme, O., Robin, A.C., & Mohan, V. 1994, A&A, 284, 810
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2003 Springer Science+Business Media Dordrecht
About this chapter
Cite this chapter
Altmann, M., de Boer, K.S., Edelmann, H. (2003). SDB Stars and the Structure of the Milky Way. In: de Martino, D., Silvotti, R., Solheim, JE., Kalytis, R. (eds) White Dwarfs. NATO Science Series, vol 105. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0215-8_16
Download citation
DOI: https://doi.org/10.1007/978-94-010-0215-8_16
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-1364-5
Online ISBN: 978-94-010-0215-8
eBook Packages: Springer Book Archive