Solar and stellar rotation
[ X ]
Tarih
2007
Yazarlar
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
Astronomical Soc Pacific
Erişim Hakkı
info:eu-repo/semantics/closedAccess
Özet
The secular evolution of the stellar rotation through angular momentum loss, driven by the stellar wind, and the consequences of the angular momentum transfers between orbit and spinning components in binary star systems will be reviewed with the special emphasis on the Solar rotation. A large co-rotating distance (Alfven radius) of the magnetically driven wind around single stars will be introduced to explain the large angular momentum loss from close binary star systems.
Açıklama
Workshop on Solar and Stellar Physics through Eclipses -- MAR 27-29, 2006 -- Ankara Univ, ORSEM Campus, Side, Antalya, TURKEY
Anahtar Kelimeler
Chromospherically Active Binaries, Orbital Period Decrease, Angular-Momentum, Kinematics, Evolution, Stars
Kaynak
Solar and Stellar Physics Through Eclipses
WoS Q Değeri
N/A
Scopus Q Değeri
Cilt
370
