A new interpretation of the low radial velocity determined from the HeII emission line in the galactic supersoft X-ray source RX J0019.8+2156

Izumi Hachisu, Mariko Kato

Research output: Contribution to journalConference article

Abstract

We propose a new interpretation for the low radial velocity of He II emission line in the Galactic supersoft X-ray source RX J0019.8+2156 based on a 2-D numerical simulation of dynamical mass transfer in binary systems. A more massive main-sequence (MS) companion of ̃ 2:0 M⊙ is derived for a ̃ 0:6 M⊙ white dwarf (WD) primary.

Original languageEnglish
Number of pages1
JournalRevista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
Volume20
Publication statusPublished - 2004 Dec 1
EventIAU Colloquium 194 - Compact Binaries in the Galaxy and Beyond - La Paz, B.C. Sur, Mexico
Duration: 2003 Nov 172003 Nov 22

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

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