Observations of AR Sco with Chandra and AstroSat soft X-ray telescope

K. P. Singh,V. Girish,J. Tiwari,P. E. Barrett,D. A. H. Buckley,S. B. Potter,E. Schlegel,V. Rana,G. Stewart

JOURNAL OF ASTROPHYSICS AND ASTRONOMY（2021）

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摘要

We present our AstroSat soft X-ray observations of a compact binary system, AR Sco, and analysis of its X-ray observations with Chandra that were taken only about a week before the AstroSat observations. An analysis of the soft X-ray (0.3–2.0 keV) data limits the modulation of the spin, orbital, or beat periods to less than 0.03 counts s ^-1 or <10

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关键词

Stars: individual: AR Sco, X-rays: binaries: novae, cataclysmic variables, white dwarfs

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