Título: The X-ray quiescence of Swift J195509.6+261406 (GRB 070610): an optical bursting X-ray binary?
Autores: Rea, Nanda
Jonker, Peter G.
Nelemans, Gijs
Pons Botella, José Antonio
Kasliwal, Mansi M.
Kulkarni, Shrinivas R.
Wijnands, Rudy
Fecha: 2013-11-14
2013-11-14
2011-02-15
Publicador: RUA Docencia
Fuente:
Tipo: info:eu-repo/semantics/article
Tema: Stars: magnetic field
X-rays: individual (SWIFT J195509.6+261406)
X-rays: stars
Astronomía y Astrofísica
Descripción: We report on an ~63 ks Chandra observation of the X-ray transient Swift J195509.6+261406 discovered as the afterglow of what was first believed to be a long-duration gamma-ray burst (GRB 070610). The outburst of this source was characterized by unique optical flares on timescales of second or less, morphologically similar to the short X-ray bursts usually observed from magnetars. Our Chandra observation was performed ~2 years after the discovery of the optical and X-ray flaring activity of this source, catching it in its quiescent state. We derive stringent upper limits on the quiescent emission of Swift J195509.6+261406, which argues against the possibility of this object being a typical magnetar. Our limits show that the most viable interpretation on the nature of this peculiar bursting source is a binary system hosting a black hole or a neutron star with a low-mass companion star (<0.12 M ☉) and with an orbital period smaller than a few hours.
N.R. is supported by a Ramón y Cajal fellowship through Consejo Superior de Investigaciones Científicas, by grants AYA2009-07391 and SGR2009-811. P.G.J. and G.N. acknowledge support from a VIDI grant from the Netherlands Organization for Scientific Research.
Idioma: Inglés

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