From a multiwavelength long term monitoring of KQ Pup, we derive a revised orbital period of 9500 days. The presence of an accreting stream is put in evidence by a large decrease of the FUV continuum due to Rayleigh scattering, and by the appearance of redshifted absorptions since Φ = 0.82.
Wind accretion in KQ Puppis / GONZALEZ RIESTRA, R; Rossi, Corinne; Viotti, R.. - STAMPA. - 261:(2002), pp. 281-282. (Intervento presentato al convegno The Physics of Cataclysmic Variables and Related Objects, tenutosi a Gottingen nel 5-10 agosto 2001).
Wind accretion in KQ Puppis
ROSSI, Corinne;
2002
Abstract
From a multiwavelength long term monitoring of KQ Pup, we derive a revised orbital period of 9500 days. The presence of an accreting stream is put in evidence by a large decrease of the FUV continuum due to Rayleigh scattering, and by the appearance of redshifted absorptions since Φ = 0.82.File allegati a questo prodotto
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