Radio pulsar and accretion regimes of rapidly rotating magnetic neutron stars in early-type eccentric binaries

Details Radio pulsar and accretion regimes of rapidly rotating magnetic neutron stars in early-type eccentric binaries Radio pulsar and accretion regimes of rapidly rotating magnetic neutron stars in early-type eccentric binaries

1994-11-16

arxiv.org/abs/astro-ph/9411064v1

Astronomy and Astrophysics

Astrophysics

accepted for publication in A&A main journal. 5 pages, latex file, laa style, no figures

Scientific paper

Rapidly rotating magnetic neutron stars in eccentric binary systems containing an early type star provide a unique opportunity to investigate the interplay between radio pulsar, stellar wind and accretion phenomena. We summarise the radio pulsar-dominated and the accretion-dominated regimes, discussing how the transition from one regime to another can take place as a result of the varying orbital distance and relative velocity along the orbit, as well as changes of the wind characteristics. We derive the conditions under which the two known B star/radio pulsar binaries (PSR 1259-63 and PSR J0045-7319) can undergo a transition to the accreting regime. A strong increase of the mass loss ouflow from the companion is required, just to cause the onset of accretion onto the magnetospheric boundary. We also show that the X--ray transient A0538-66 is likely to undergo transitions from the accreting neutron star regime, to the regime of accretion onto the magnetosphere. These two regimes might correspond to the high (> 10^{38} erg/s) and the low-luminosity (< 10^{38} erg/s) outbursts observed from this source. A radio pulsar might become detectable in the long quiescent states of A0538-66. A new model of the enigmatic high-energy binary LS I +61 303 involving accretion onto the magnetosphere is also presented.

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