0125241 - ASU-R 20030147 RIV NL eng J - Článek v odborném periodiku
Kubát, Jiří - Krtička, Jiří - Pustylnik, I. B.
Radiation induced coronal wind in late B stars.
New Astronomy. Roč. 9, č. 3 (2004), s. 215-224. ISSN 1384-1076. E-ISSN 1384-1092
Grant CEP: GA ČR GA205/01/0656; GA ČR GA205/02/0445; GA AV ČR KSK2043105
Výzkumný záměr: CEZ:AV0Z1003909
Klíčová slova: early type stars * coronae stars * hydrodynamics
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 2.171, rok: 2004

Multicomponent radiatively driven winds in the late B stars cause significant heating of the layers just above the photosphere. These heated layers form a hot region - a corona, which may provide a significant fraction of energy necessary for the formation of a coronal wind driven by gas pressure.
Trvalý link: http://hdl.handle.net/11104/0023498