A new clue to the transition mechanism between optical high and low states of the supersoft X-ray source RX J0513.9-6951, implied by the recurrent nova CI aquilae 2000 outburst model

Izumi Hachisu, Mariko Kato

Research output: Contribution to journalArticle

40 Citations (Scopus)

Abstract

We have found a new clue to the transition mechanism between optical high/X-ray off and optical low/X-ray on states of the LMC supersoft X-ray source RX J0513.9-6951. A sharp ∼1 mag drop is common to the CI Aql 2000 outburst. These drops are naturally attributed to the cessation of optically thick winds on white dwarfs. A detailed light-curve analysis of CI Aql indicates that the size of a disk drastically shrinks when the wind stops. This causes a ∼1-2 mag drop in the optical light curve. In RX J0513.9-6951, the same mechanism reproduces sharp ∼1 mag drop from optical high to low states. We predict that this mechanism also works on the transition from low to high states. Interaction between the wind and the companion star attenuates the mass transfer and drives full cycles of low and high states.

Original languageEnglish
Pages (from-to)1003-1008
Number of pages6
JournalAstrophysical Journal
Volume588
Issue number2 I
DOIs
Publication statusPublished - 2003 May 10

Fingerprint

outburst
light curve
x rays
companion stars
mass transfer
cycles
causes
interactions
analysis

Keywords

  • Binaries: close
  • Novae, cataclysmic variables
  • Stars : individual (CI Aquilae, RX J0513.9-6951)
  • Stars: winds, outflows
  • X-rays: stars

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

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title = "A new clue to the transition mechanism between optical high and low states of the supersoft X-ray source RX J0513.9-6951, implied by the recurrent nova CI aquilae 2000 outburst model",
abstract = "We have found a new clue to the transition mechanism between optical high/X-ray off and optical low/X-ray on states of the LMC supersoft X-ray source RX J0513.9-6951. A sharp ∼1 mag drop is common to the CI Aql 2000 outburst. These drops are naturally attributed to the cessation of optically thick winds on white dwarfs. A detailed light-curve analysis of CI Aql indicates that the size of a disk drastically shrinks when the wind stops. This causes a ∼1-2 mag drop in the optical light curve. In RX J0513.9-6951, the same mechanism reproduces sharp ∼1 mag drop from optical high to low states. We predict that this mechanism also works on the transition from low to high states. Interaction between the wind and the companion star attenuates the mass transfer and drives full cycles of low and high states.",
keywords = "Binaries: close, Novae, cataclysmic variables, Stars : individual (CI Aquilae, RX J0513.9-6951), Stars: winds, outflows, X-rays: stars",
author = "Izumi Hachisu and Mariko Kato",
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T1 - A new clue to the transition mechanism between optical high and low states of the supersoft X-ray source RX J0513.9-6951, implied by the recurrent nova CI aquilae 2000 outburst model

AU - Hachisu, Izumi

AU - Kato, Mariko

PY - 2003/5/10

Y1 - 2003/5/10

N2 - We have found a new clue to the transition mechanism between optical high/X-ray off and optical low/X-ray on states of the LMC supersoft X-ray source RX J0513.9-6951. A sharp ∼1 mag drop is common to the CI Aql 2000 outburst. These drops are naturally attributed to the cessation of optically thick winds on white dwarfs. A detailed light-curve analysis of CI Aql indicates that the size of a disk drastically shrinks when the wind stops. This causes a ∼1-2 mag drop in the optical light curve. In RX J0513.9-6951, the same mechanism reproduces sharp ∼1 mag drop from optical high to low states. We predict that this mechanism also works on the transition from low to high states. Interaction between the wind and the companion star attenuates the mass transfer and drives full cycles of low and high states.

AB - We have found a new clue to the transition mechanism between optical high/X-ray off and optical low/X-ray on states of the LMC supersoft X-ray source RX J0513.9-6951. A sharp ∼1 mag drop is common to the CI Aql 2000 outburst. These drops are naturally attributed to the cessation of optically thick winds on white dwarfs. A detailed light-curve analysis of CI Aql indicates that the size of a disk drastically shrinks when the wind stops. This causes a ∼1-2 mag drop in the optical light curve. In RX J0513.9-6951, the same mechanism reproduces sharp ∼1 mag drop from optical high to low states. We predict that this mechanism also works on the transition from low to high states. Interaction between the wind and the companion star attenuates the mass transfer and drives full cycles of low and high states.

KW - Binaries: close

KW - Novae, cataclysmic variables

KW - Stars : individual (CI Aquilae, RX J0513.9-6951)

KW - Stars: winds, outflows

KW - X-rays: stars

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