The neutron star transient XTE J1701-407 has returned to quiescence after a 3-year long outburst

Bibcode
2011ATel.3604....1D
Degenaar, N.; Wijnands, R.; Altamirano, D.; Cackett, E.; Linares, M.; Homan, J.; Fridriksson, J.
Referencia bibliográfica

The Astronomer's Telegram, #3604

Fecha de publicación:
8
2011
Número de autores
7
Número de autores del IAC
0
Número de citas
3
Número de citas referidas
2
Descripción
The neutron star low-mass X-ray binary and long thermonuclear burst source XTE J1701-407 (ATel #1618) has been active ever since its discovery in 2008 June (ATel #1569), displaying a typical 2-10 keV luminosity of ~5E36 erg/s (assuming a distance D=5.0 kpc; ATel #2814). However, routine monitoring of the Galactic bulge with the PCA aboard RXTE (Swank & Markwardt 2001, ASP conference series 251, 94) indicates that the outburst has now ceased: the source intensity has remained below the detection limit of the PCA since 2011 August 9 (see the link provided below).
Tipo
Sin árbitro

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