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À propos de : Supergiant, fast, but not so transient 4U 1907+09        

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  • Supergiant, fast, but not so transient 4U 1907+09
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  • We have investigated the dipping activity observed in the high-mass X-ray binary 4U 1907+09 and shown that the source continues to pulsate in the “off” state, noting that the transition between the “on” and “off” states may be either dip-like or flare-like. This behavior may be explained in the framework of the “gated accretion” scenario proposed to explain the flares in supergiant fast X-ray transients (SFXTs). We conclude that 4U 1907 + 09 might prove to be a missing link between the SFXTs and ordinary accreting pulsars.
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  • aa20085-12
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  • © ESO, 2012
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  • ESO
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