Journal of Astronomy and Space Sciences

The Korean Space Science Society (한국우주과학회)
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The Vertical Structure of Accretion Disks for Dwarf Novae

왜신성에 대한 Accretion Disk의 수직구조

  • Kyu Hong Choi (Department of Astronomy & Meteorolgy, Yonsei University) ;
  • Kyung Mee Kim (Department of Astronomy & Meteorolgy, Yonsei University)
  • Published : 1985.06.01
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Abstract

We have constructed models of steady accretion disk with accretion rate M=$10^{16}g/sec$ or $10^{18}g/sec$. The mass of the radius of white dwarf were taken as $1M_\odot$ and $10^9cm$, respectively. The possible application of the results to Z Cha and Z Cam are discussed.

Accretion rate가 $M=10^{16}g/sec$ 와 $M=10^{18}g/sec$인 경우의 정상상태의 Accretion disk의 모델들을 만들었다. 중심에 있는 별은 백색왜성으로 가정하고 질량은 $1M_\odot$이고 반경은 $10^9cm$로 보았다. 이 모델을 왜신성인 Z cha와 Z Cam에 응용하였다.

Keywords