Autor:	R. J. Dickinson, R. K. Prinja, S. R. Rosen, K. Horne
Rok vydání:	1996
Zdroj:	International Astronomical Union Colloquium. 158:41-42
ISSN:	0252-9211
DOI:	10.1017/s0252921100038161
Popis:	We present high resolution optical spectroscopy of the cataclysmic variable (CV) V795 Her. The time- and phase- dependent behaviour of the emission source is examined using two-dimensional image analysis and Doppler reconstruction techniques on the orbital profiles. A clear S-wave modulation of a weak emission feature in the Hβ and Hγ line wings (extending to ~1800 km s−1) is present, with complex asymmetric properties.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::ca7666645e47f248c65c04e885205d00 https://doi.org/10.1017/s0252921100038161 Zobrazit plný text záznamu