Amanote Research
Register
Sign In
Hot Subdwarf Stars in Close-Up View
Astronomy and Astrophysics
- France
doi 10.1051/0004-6361/201220549
Full Text
Open PDF
Abstract
Available in
full text
Categories
Astrophysics
Astronomy
Planetary Science
Space
Date
January 1, 2013
Authors
S. Geier
Publisher
EDP Sciences
Related search
Asteroseismology of Hot B Subdwarf Stars
EPJ Web of Conferences
Astronomy
Physics
Why Do Hot Subdwarf Stars Pulsate?
Proceedings of the International Astronomical Union
Astrophysics
Astronomy
Planetary Science
Space
New Advances in Asteroseismology of Pulsating Hot Subdwarf Stars
Proceedings of the International Astronomical Union
Astrophysics
Astronomy
Planetary Science
Space
G-Mode Trapping and Period Spacings in Hot B Subdwarf Stars
Proceedings of the International Astronomical Union
Astrophysics
Astronomy
Planetary Science
Space
A Search for Hot Subdwarf Companions to Rapidly-Rotating Early B Stars
Proceedings of the International Astronomical Union
Astrophysics
Astronomy
Planetary Science
Space
Probing the Driving Region in Hot Subdwarf Stars Through Nonadiabatic Asteroseismology: The Principle of the Method
Astronomy and Astrophysics
Astrophysics
Astronomy
Planetary Science
Space
A Close-Up View of Codon Selection in Eukaryotic Initiation
RNA Biology
Cell Biology
Molecular Biology
Hot Subdwarf Binaries From the MUCHFUSS Project
Astronomy and Astrophysics
Astrophysics
Astronomy
Planetary Science
Space
The First Ultracompact Roche Lobe–Filling Hot Subdwarf Binary
Astrophysical Journal
Astrophysics
Astronomy
Planetary Science
Space