Change the language. The current language is:
English
Spanish
Register
Login
Current issue
Previous issues
About
About RMxAC
Editorial Team
Privacy Statement
Contact
Authors and editors instructions
Search
RmXAA
Register
Login
Change the language. The current language is:
English
Spanish
Vol. 40 No. 1 (2011)
,
Contributions
Vol. 40 No. 1 (2011)
Contributions
The structure of BB Doradus in quiescence
Schmidtobreick L.
+
−
Rodríguez-Gil P.
+
−
Long K. S.
+
−
Gänsicke B. T.
+
−
Tappert C.
+
−
Schmidtobreick L.
European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile.
Rodríguez-Gil P.
-
Long K. S.
-
Gänsicke B. T.
-
0000-0002-2761-3005
Tappert C.
-
PDF
PDF
Keywords
accretion
accretion disks
stars: activity
stars: magnetic field
stars: variables: general
How to Cite
The structure of BB Doradus in quiescence. (2011).
Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias
,
40
(1), 288-288.
https://astronomia.unam.mx/journals/rmxac/article/view/2011rmxac..40..288s
hola
More Citation Formats
ACM
ACS
APA
ABNT
Chicago
Harvard
IEEE
MLA
Turabian
Vancouver
AMA
Download Citation
Endnote/Zotero/Mendeley (RIS)
BibTeX
Abstract
Spectroscopic observations during a low state of BB Dor reveal a complex emission distribution. Irradiation by the white dwarf as well as magnetic fields of the secondary star are needed for an explanation.
×
Username
*
Required
Password
*
Required
Forgot your password?
Keep me logged in
Login
No account?
Register here