A strongly magnetic neutron star in a nearly face-on binary system

P. Daumerie, V. Kalogera, F. K. Lamb, Dimitrios Psaltis

Research output: Contribution to journalArticle

27 Citations (Scopus)

Abstract

THE first example of a new type of transient X-ray source recently appeared in the direction of the Galactic Centre. During the peak of its outburst, the new source, GRO J1744-28, was very bright in X-rays and produced both 2.1-Hz periodic pulsations and intense bursts lasting tens of seconds. Before the discovery of this source, it was thought that X-ray stars could not display these different types of activity simultaneously. Here we discuss the nature of the source, which seems to be a strongly magnetic neutron star accreting matter from a low-mass companion star in a low- inclination orbit. The dipole component of its magnetic field is λ 1011 G. When the source was at its brightest, its X-ray luminosity between bursts was close to the Eddington critical luminosity, at which the outward force of the escaping radiation balances the inward force of gravity. The X-ray bursts probably occur when matter that has accumulated in the inner part of the accretion disk briefly overcomes the forces that oppose its inflow, and the gas falls onto the neutron star.

Original languageEnglish (US)
Pages (from-to)141-143
Number of pages3
JournalNature
Volume382
Issue number6587
DOIs
StatePublished - 1996
Externally publishedYes

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magnetic stars
neutron stars
bursts
x rays
luminosity
companion stars
accretion disks
inclination
gravitation
dipoles
orbits
stars
radiation
gases
magnetic fields

ASJC Scopus subject areas

  • General

Cite this

A strongly magnetic neutron star in a nearly face-on binary system. / Daumerie, P.; Kalogera, V.; Lamb, F. K.; Psaltis, Dimitrios.

In: Nature, Vol. 382, No. 6587, 1996, p. 141-143.

Research output: Contribution to journalArticle

Daumerie, P, Kalogera, V, Lamb, FK & Psaltis, D 1996, 'A strongly magnetic neutron star in a nearly face-on binary system', Nature, vol. 382, no. 6587, pp. 141-143. https://doi.org/10.1038/382141a0
Daumerie, P. ; Kalogera, V. ; Lamb, F. K. ; Psaltis, Dimitrios. / A strongly magnetic neutron star in a nearly face-on binary system. In: Nature. 1996 ; Vol. 382, No. 6587. pp. 141-143.
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