The pre-outburst flare of the A 0535+26 August/September 2005 outburst

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https://www.aanda.org/articles/aa/abs/2008/11/aa9310-07/aa9310-07.html

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https://doi.org/10.1051/0004-6361:20079310
 http://hdl.handle.net/11603/29957

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UMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
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UMBC Physics Department

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https://orcid.org/0000-0002-4656-6881

Date

2008-01-25

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journal articles
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Citation of Original Publication

Caballero, I., A. Santangelo, P. Kretschmar, R. Staubert, K. Postnov, D. Klochkov, A. Camero-Arranz, et al. “The Pre-Outburst Flare of the A 0535+26 August/September 2005 Outburst.” Astronomy & Astrophysics 480, no. 2 (March 1, 2008): L17–20. https://doi.org/10.1051/0004-6361:20079310.

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Abstract

Aims.We study the spectral and temporal behavior of the High Mass X-ray Binary A 0535+26 during a “pre-outburst flare” which took place ~ 5 d before the peak of a normal (type I) outburst in August/September 2005. We compare the studied behavior with that observed during the outburst. Methods.We analyse RXTEobservations that monitored A 0535+26 during the outburst. We complete spectral and timing analyses of the data. We study the evolution of the pulse period, present energy-dependent pulse profiles both at the initial pre-outburst flare and close to outburst maximum, and measure how the cyclotron resonance-scattering feature (hereafter CRSF) evolves. Results.We present three main results: a constant period P = 103.3960(5) sis measured until periastron passage, followed by a spin-up with a decreasing period derivative of P= (-1.69 ±0.04) 10⁻⁸ ss⁻¹ at MJD 53 618, and P remains constant again at the end of the main outburst. The spin-up provides evidence for the existence of an accretion disk during the normal outburst. We measure a CRSF energy of E꜀ᵧ꜀~ 50 keV during the pre-outburst flare, and E꜀ᵧ꜀ ~ 46 keV during the main outburst. The pulse shape, which varies significantly during both pre-outburst flare and main outburst, evolves strongly with photon energy.