Discovery of kilohertz QPOs in RXTE observations of SAX J1748.9-2021.

Altamirano, D.; Patruno, A.; Watts, A.; Armas Padilla, M.; Cavecchi, Y.; Degenaar, N.; Kalamkar, M.; Kaur, R.; Soleri, P.; Yang, Y. J.; van der Klis, M.; Wijnands, R.; Casella, P.; Linares, M.; Rea, N.
Referencia bibliográfica

The Astronomer's Telegram, #2426

Fecha de publicación:
2
2010
Número de autores
15
Número de autores del IAC
0
Número de citas
9
Número de citas referidas
7
Descripción
We report on RXTE observations of the ongoing outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021 (Altamirano et al. 2008, 674, 45A, see ATEL #2360 and #2407). Since the first detection of intermittent pulsations on January 27th, 2010, observations have been carried out on a daily basis. The source remained between 120 and 160 mCrab (2-16 keV - see ATEL #2407) until February 3rd, when the intensity started to decrease.