Flares in the X-ray source EXO 2030 + 375

Details Flares in the X-ray source EXO 2030 + 375 Flares in the X-ray source EXO 2030 + 375

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...375..701a&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 375, July 10, 1991, p. 701-703.

Astronomy and Astrophysics

Astrophysics

6

B Stars, Stellar Flares, X Ray Binaries, X Ray Sources, Rayleigh Waves, Satellite Observation, Taylor Instability

Scientific paper

Six X-ray flares were observed in the source EXO 2030 + 375 with an
average time interval of about 4 hr between the flares. It is shown here
that the flares can be due to Rayleigh-Taylor instabilities near the
magnetospheric boundary of the neutron star when it reaches the
equilibrium period.

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