Infrared bursts from Liller I/MXB 1730-333

Details Infrared bursts from Liller I/MXB 1730-333 Infrared bursts from Liller I/MXB 1730-333

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..127a&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 1, Sept. 1980, p. 127-132.

Astronomy and Astrophysics

Astronomy

3

Bursts, Cyclotron Radiation, Globular Clusters, Infrared Astronomy, Stellar Models, X Ray Sources, Binary Stars, Magnetohydrodynamic Waves, Masers, Neutron Stars, Periodic Variations, Radiant Flux Density, Radii, Stellar Magnetic Fields, Stellar Mass Accretion

Scientific paper

The observation of infrared bursts from the globular cluster Liller I has been reported by Kulkarni et al. (1979) and confirmed by Jones et at. (1980). The infrared bursts which resemble Type I X-ray bursts in their characteristics are plausibly attributed to a cyclotron maser instability operating at few tens of neutron star radii above the poles of a magnetized neutron star in a binary system. It is suggested that similar infrared bursts should in general be observable from Type I X-ray burst sources.

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