The reawakening of the sleeping X-ray pulsar XTE J1946+274

Müller S, Kühnel M, Caballero I, Pottschmidt K, Fürst F, Kreykenbohm I, Sagredo M, Obst M, Wilms J, Ferrigno C, Rothschild RE, Staubert R (2012)


Publication Status: Published

Publication Type: Journal article

Publication year: 2012

Journal

Publisher: EDP SCIENCES S A

Book Volume: 546

Article Number: ARTN A125

DOI: 10.1051/0004-6361/201219580

Abstract

We report on a series of outbursts of the high-mass X-ray binary XTE J1946+274 in 2010/2011 observed with INTEGRAL, RXTE, and Swift. We discuss possible mechanisms resulting in the extraordinary outburst behavior of this source. The X-ray spectra can be described by standard phenomenological models, enhanced by an absorption feature of unknown origin at about 10 keV and a narrow iron K alpha fluorescence line at 6.4 keV, which are variable in flux and pulse phase. We find possible evidence for a cyclotron resonance scattering feature at about 25 keV at the 93% level. The presence of a strong cyclotron line at 35 keV seen in data from the source's 1998 outburst that was confirmed by a reanalysis of these data can be excluded. This result indicates that the cyclotron line feature in XTE J1946+274 is variable between individual outbursts.

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APA:

Müller, S., Kühnel, M., Caballero, I., Pottschmidt, K., Fürst, F., Kreykenbohm, I.,... Staubert, R. (2012). The reawakening of the sleeping X-ray pulsar XTE J1946+274. Astronomy & Astrophysics, 546. https://doi.org/10.1051/0004-6361/201219580

MLA:

Müller, Sebastian, et al. "The reawakening of the sleeping X-ray pulsar XTE J1946+274." Astronomy & Astrophysics 546 (2012).

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