Swift observations of SAX J1808.4-3658

Monitoring the return to quiescence

Sergio Campana, Luigi Stella, Jamie A. Kennea

Research output: Contribution to journalArticle

37 Citations (Scopus)

Abstract

The transient accreting millisecond pulsar SAX J1808.4-3658 has shown several outbursts to date but the transition from outburst to quiescence has never been investigated in detail. Thanks to the Swift observing flexibility, we monitored for the first time the decay to quiescence during the 2005 outburst. At variance with other transients, wide luminosity variations are observed. In addition, close to quiescence, SAX J1808.4-3658 seems to switch between two different states. We interpret them in terms of the accretion states accessible to a magnetized, fast-rotating neutron star.

Original languageEnglish (US)
JournalAstrophysical Journal
Volume684
Issue number2 PART 2
DOIs
StatePublished - Jan 1 2008

Fingerprint

outburst
pulsars
neutron stars
flexibility
switches
luminosity
decay
monitoring
accretion

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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abstract = "The transient accreting millisecond pulsar SAX J1808.4-3658 has shown several outbursts to date but the transition from outburst to quiescence has never been investigated in detail. Thanks to the Swift observing flexibility, we monitored for the first time the decay to quiescence during the 2005 outburst. At variance with other transients, wide luminosity variations are observed. In addition, close to quiescence, SAX J1808.4-3658 seems to switch between two different states. We interpret them in terms of the accretion states accessible to a magnetized, fast-rotating neutron star.",
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Swift observations of SAX J1808.4-3658 : Monitoring the return to quiescence. / Campana, Sergio; Stella, Luigi; Kennea, Jamie A.

In: Astrophysical Journal, Vol. 684, No. 2 PART 2, 01.01.2008.

Research output: Contribution to journalArticle

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AU - Campana, Sergio

AU - Stella, Luigi

AU - Kennea, Jamie A.

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