Emission Line Analyses of HBV 475, V1016 CYG, and HM SGE
نویسندگان
چکیده
منابع مشابه
Raman Scattered O Vi Λ 6825 and the Accretion Disk Emission Model in the Symbiotic Stars V1016 Cygni and Hm Sagittae
We present the high resolution spectra of the D type symbiotic stars V1016 Cygni and HM Sagittae obtained with the Bohyunsan Optical Echelle Spectrograph (BOES), and investigate the doublepeaked asymmetric profiles of the Raman scattered O VI 6825. This feature is formed through Raman scattering of O VI 1032 by atomic hydrogen with small scattering cross section of ∼ 10 cm, requiring a specific...
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ژورنال
عنوان ژورنال: International Astronomical Union Colloquium
سال: 1988
ISSN: 0252-9211
DOI: 10.1017/s0252921100103641