Evento
Multiwavelength monitoring of a very active dwarf nova AX J1549.8-5416 with an unusually high duty cycle
Zhang, Guobao; Gelfand, Joseph D.; Russell, David M.; Lewis, Fraser; Masetti, Nicola; Bernardini, Federico; Andruchow, Ileana
; Zibecchi, Lorena Cecilia
Colaboradores:
Arnaud, M.
Tipo del evento:
Simposio
Nombre del evento:
The X-ray Universe 2017
Fecha del evento:
06/06/2017
Institución Organizadora:
European Space Agency;
XMM Newton Science Center;
National Institute for Astrophysics;
Italian Space Agency;
University Roma Tre;
La Sapienza University;
Título del Libro:
Monthly Notices of the Royal Astronomical Society
Editorial:
The Royal Astronomical Society
ISSN:
1365-2966
e-ISSN:
0035-8711
Idioma:
Inglés
Clasificación temática:
Resumen
We present new optical, UV and X-ray observations of a highly variable dwarf nova(DN) AX J1549.8-5416. The multiwavelength analysis of three mini-outbursts and one normal outburst represent one of the most complete multiwavelength studies of a DN and help to refine the relationship between the X-ray, UV and optical emission in this system. We find that the UV emission is delayed the optical (1.0-5.4 days) during the rising phase of the outburst. The X-ray emission is suppressed during the peak of the optical outburst and recovers during the end of the outburst. We also analyse archival Swift, Chandra and XMM-Newton observations of the source. Our estimated high duty cycle suggests the X-ray luminosity of this source should be larger than 10E32 erg/s in quiescence. We find a roughly anti-correlation between X-ray and UV flux. The X-ray spectra of XMM-Newton and Chandra can be well described either by a single temperature thermal plasma model or by an isobaric cooling flow model when its X-ray flux is high.
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Eventos de INST.DE ASTROFISICA LA PLATA
Citación
Multiwavelength monitoring of a very active dwarf nova AX J1549.8-5416 with an unusually high duty cycle; The X-ray Universe 2017; Roma; Italia; 2017; 1-13
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