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

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

外国語・総合教育教室

研究成果: Conference article › 査読

抄録

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.

本文言語	English
ページ数	1
ジャーナル	Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
巻	20
出版ステータス	Published - 2004 12月 1
イベント	IAU Colloquium 194 - Compact Binaries in the Galaxy and Beyond - La Paz, B.C. Sur, Mexico 継続期間: 2003 11月 17 → 2003 11月 22

ASJC Scopus subject areas

宇宙惑星科学
天文学と天体物理学

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引用スタイル

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title = "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",

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.",

author = "Izumi Hachisu and Mariko Kato",

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T1 - 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

AU - Hachisu, Izumi

AU - Kato, Mariko

PY - 2004/12/1

Y1 - 2004/12/1

N2 - 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.

AB - 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.

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M3 - Conference article

AN - SCOPUS:70649107118

SN - 1405-2059

VL - 20

JO - Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

JF - Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

T2 - IAU Colloquium 194 - Compact Binaries in the Galaxy and Beyond

Y2 - 17 November 2003 through 22 November 2003

ER -