Number of the records: 1
Radiation induced coronal wind in late B stars
- 1.
SYSNO ASEP 0125241 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Ostatní články Title Radiation induced coronal wind in late B stars Author(s) Kubát, Jiří (ASU-R) RID, ORCID
Krtička, Jiří (ASU-R)
Pustylnik, I. B. (EE)Source Title New Astronomy. - : Elsevier - ISSN 1384-1076
Roč. 9, č. 3 (2004), s. 215-224Number of pages 10 s. Language eng - English Country NL - Netherlands Keywords early type stars ; coronae stars ; hydrodynamics Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects GA205/01/0656 GA ČR - Czech Science Foundation (CSF) GA205/02/0445 GA ČR - Czech Science Foundation (CSF) KSK2043105 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) CEZ AV0Z1003909 - ASU-R Annotation 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. Workplace Astronomical Institute Contact Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2004
Number of the records: 1