RXTE Studies of Cyclotron Lines in Accreting Pulsars

Department

Program

Citation of Original Publication

W. A. Heindl, W. Coburn, D. E. Gruber, M. Pelling, R. E. Rothschild, P. Kretschmar, I. Kreykenbohm, J. Wilms, K. Pottschmidt, R. Staubert; RXTE studies of cyclotron lines in accreting pulsars. AIP Conf. Proc. 12 April 2000; 510 (1): 178–182. https://doi.org/10.1063/1.1303198

Rights

This article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing. This article appeared in W. A. Heindl, W. Coburn, D. E. Gruber, M. Pelling, R. E. Rothschild, P. Kretschmar, I. Kreykenbohm, J. Wilms, K. Pottschmidt, R. Staubert; RXTE studies of cyclotron lines in accreting pulsars. AIP Conf. Proc. 12 April 2000; 510 (1): 178–182. https://doi.org/10.1063/1.1303198 and may be found at https://pubs.aip.org/aip/acp/article-abstract/510/1/178/559181/RXTE-studies-of-cyclotron-lines-in-accreting.

Subjects

Abstract

In this paper, we summarize the RXTE measurements of cyclotron resonance scattering features in 8 accreting pulsars. The wide bandpass and modest resolution of the RXTE instruments make them ideal for measuring these generally broad features. In particular, the high energy response of HEXTE provides a window for discovery of new lines not detectable with proportional counters such as Ginga or the PCA alone.