AbstractWe discuss the X-ray line emission as observed with the HETG on Chandra of a sample of CV spectra. A portion of the data have been fit with global models by Mukai et al. [Mukai, K. et al. Two types of X-ray spectra in cataclysmic variables. ApJ 586, L77–L80, 2003]; we analyze the same spectra using a line-by-line fit. The results are similar to those reported by Mauche et al. on EX Hya, but additionally cover the other CVs. A broad range of temperatures is indicated based on the H/He-like ratio of O, Mg, S, and Fe.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    X-ray line emission from cataclysmic variables


    Beteiligte:
    Schlegel, E.M. (Autor:in) / Singh, K.P. (Autor:in) / Rana, V. (Autor:in) / Barrett, P. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 40 , 8 ; 1299-1302


    Erscheinungsdatum :

    2006-10-30


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




    X-ray line emission from cataclysmic variables

    Schlegel, E.M. | Online Contents | 2007


    Winds from Cataclysmic Variables

    Kallman, T. | NTRS | 1988


    Winds from cataclysmic variables

    Kallman, T. | Elsevier | 1988


    A Comprehensive Study of X-ray Emission Lines from Cataclysmic Variables

    Singh, K. P. / Rana, V. R. / Schlegel, E. M. et al. | British Library Conference Proceedings | 2005


    Hard X-ray cataclysmic variables

    de Martino, D. / Bernardini, F. / Mukai, K. et al. | Elsevier | 2019