Hydrogen deficient donors in low-mass X-ray binaries

Simple item page
dc.creatorNelemans, Gijs
dc.date2007-11-05
dc.date.accessioned2026-07-07T08:40:41Z
dc.date.available2026-07-07T08:40:41Z
dc.descriptionA number of X-ray binaries (neutron stars or black holes accreting from a companion star) have such short orbital periods that ordinary, hydrogen rich, stars do not fit in. Instead the mass-losing star must be a compact, evolved star, leading to the transfer of hydrogen deficient material to the neutron star. I discuss the current knowledge of these objects, with focus on optical spectroscopy.
dc.descriptionin proceedings "Hydrogen-Deficient Stars" (eds. K Werner & T Rauch), ASP Conf Series
dc.identifierhttps://arxiv.org/abs/0711.0602
dc.identifierhttp://arxiv.org/abs/0711.0602
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/141443
dc.subjectAstrophysics
dc.titleHydrogen deficient donors in low-mass X-ray binaries
dc.typetext

Files

Collections

arXiv