X-RAY RADIATIONS OF INTERACTING BINARY 44i BOOTIS

  • KIM YONGGI (Dept. of Astronomy & Space Science, Chungbuk National University) ;
  • KIM MINSU (Dept. of Astronomy & Space Science, Chungbuk National University)
  • Published : 1996.12.01

Abstract

In order to study the X-ray radiations from solar type strong interacting binary stars, we have collected X-ray data of 44i Bootis (P=0.2678 days, SP=G2+G2) from the EXOSAT data archive. Preliminarly analysis of a part of these data has been already reported by Vilhu & Heise (1986). In this paper, however, we present a more complete light curve in LE region than the previous work, and some unpublished X-ray light curves and spectrums. Using these new materials a new attempt to find the physical explanation about. some observational characteristic figures in the X-ray light curves and spectrums has been made.

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