PUSKULLU, Caglar, Faruk SOYDUGAN and Jiří KRTIČKA. Secilmis bazi sicak yildizlarin HST morote tayflarinda P Cygni profilleri (P Cygni line profiles of stellar wind observed by HST). Canakkale, Turecko: Canakkale Onsekiz Mart Universitesi, 2008, 4 pp. Ulusal astronomi kongresi. ISBN 9758100335.
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Basic information
Original name Secilmis bazi sicak yildizlarin HST morote tayflarinda P Cygni profilleri
Name in Czech P Cygni profily hvezdneho vetru pozorovane HST
Name (in English) P Cygni line profiles of stellar wind observed by HST
Authors PUSKULLU, Caglar, Faruk SOYDUGAN and Jiří KRTIČKA.
Edition Canakkale, Turecko, 4 pp. Ulusal astronomi kongresi, 2008.
Publisher Canakkale Onsekiz Mart Universitesi
Other information
Original language Turkish
Type of outcome Book on a specialized topic
Field of Study 10308 Astronomy
Country of publisher Turkey
Confidentiality degree is not subject to a state or trade secret
Organization unit Faculty of Science
ISBN 9758100335
Keywords in English P Cygni profiles, hot star winds, HST
Tags International impact
Changed by Changed by: prof. Mgr. Jiří Krtička, Ph.D., učo 8714. Changed: 31/10/2008 20:19.
Abstract
HST veritabanindan secilen bazi sicak yildizlarin morote tayflari, yildiz ruzgar etkilerini belirlemek ve karsilastirmak amaciyla incelendi. Ruzgara dogrudan gozlemsel kanit sunan P Cygni profilleri, belirli bazi rezonans cizgileri baz alinarak arandi. Calisilan yildizlarda ruzgarin yildizin isinim gucune ve sicakligina bagliliklari arastirildi.
Abstract (in Czech)
Ultrafialova spektra ziskana pomoci HST byla studovana pro vybrane hvezdy. P Cygni profily rezonancnich car byly povazovany jako dukaz existence vetru. Je studovan vztah mezi hvezdnym vetrem a luminozitnim typem.
Abstract (in English)
Ultraviolet spectra obtained by HST were examined for some selected hot stars to determine and compare the effects of hot stellar wind in our samples have different properties. P Cygni profiles in resonance lines were investigated as a disctinct evidence for hot stars winds. A relationship between stellar winds and spectral type-luminosity was given.
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