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20 April 2024
 
  » arxiv » 1409.5035

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NuSTAR Discovery of a Cyclotron Line in the Be/X-ray Binary RX J0520.5-6932 During Outburst
Shriharsh P. Tendulkar ; Felix Fürst ; Katja Pottschmidt ; Matteo Bachetti ; Varun B. Bhalerao ; Steven E. Boggs ; Finn E. Christensen ; William W. Craig ; Charles A. Hailey ; Fiona A. Harrison ; Daniel Stern ; John A. Tomsick ; Dominic J. Walton ; William Zhang ;
Date Wed, 17 Sep 2014 15:42:08 GMT (1867kb,D)
AbstractWe present spectral and timing analysis of NuSTAR observations of RX J0520.5$-$6932 in the 3-79 keV band collected during its outburst in January 2014. The target was observed on two epochs and we report the detection of a cyclotron resonant scattering feature with central energies of $E_mathrm{CRSF} = 31.3_{-0.7}^{+0.8}$ keV and $31.5_{-0.6}^{+0.7}$ keV during the two observations, respectively, corresponding to a magnetic field of $B approx 2 imes10^{12}$ G. The 3-79 keV luminosity of the system during the two epochs assuming a nominal distance of 50 kpc was $3.667pm0.007 imes 10^{38},mathrm{erg,s^{-1}}$ and $3.983pm0.007 imes10^{38},mathrm{erg,s^{-1}}$. Both values are much higher than the critical luminosity of $approx1.5 imes10^{37},mathrm{erg,s^{-1}}$ above which a radiation dominated shock front may be expected. This adds a new object to the sparse set of three systems that have a cyclotron line observed at luminosities in excess of $10^{38},mathrm{erg,s^{-1}}$. A broad ($sigmaapprox0.45$ keV) Fe emission line is observed in the spectrum at a central energy of $6.58_{-0.05}^{+0.05}$ keV in both epochs. The pulse profile of the pulsar was observed to be highly asymmetric with a sharply rising and slowly falling profile of the primary peak. We also observed minor variations in the cyclotron line energy and width as a function of the rotation phase.% As in observations of other cyclotron absorption line sources, there is a small ($Deltaphilesssim0.1$) phase difference between the peak of the cyclotron energy variation and the peak of the flux variation.
Source arXiv, 1409.5035
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