Constraints on the Thickness of be Star Disks Derived from Combined IR Excess and Optical Polarimetry Data-Reference-Cited by-同舟云学术

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Constraints on the Thickness of be Star Disks Derived from Combined IR Excess and Optical Polarimetry Data

Published:1990 Issue: Volume: Page:185-190
ISSN:
Container-title:Angular Momentum and Mass Loss for Hot Stars
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Author:

Bjorkman J. E.,Cassinelli J. P.

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-009-2105-4_19.pdf

Reference10 articles.

1. Bjorkman, J.E., and Cassinelli, J.P. (1990), (in preparation).

2. Bjorkman, K.S. (1989), University of Colorado Ph.D. Thesis.

3. Brown, J.C., and McLean, I.S. (1979), Astron. Astrophys. 57, 149.

4. Cassinelli, J.P., Nordsieck, K.H., and Murison, M.A. (1987), Astrophys. J. 317, 290.

5. Coté, J. and Waters, L.B.F.M. (1987), Astron. Astrophys. 176, 93.

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A Magnetically Torqued Disk Model for Be Stars;The Astrophysical Journal;2002-10-20

2. A Useful Approximation for Computing the Continuum Polarization of Be Stars;The Astrophysical Journal;2001-06

3. Deriving the Geometry of Be Star Circumstellar Envelopes from Continuum Spectropolarimetry. I. The Case of ζ Tauri;The Astrophysical Journal;1997-03-10

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