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Flares in the X-ray source EXO 2030 + 375Six 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.
Document ID
19910059760
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/170235
Authors
Apparao, Krishna M. V. (Pennsylvania State University University Park, United States)
Date Acquired
August 15, 2013
Publication Date
July 10, 1991
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 375
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
91A44383
Funding Number(s)
CONTRACT_GRANT: NAG5-941
Distribution Limits
Public
Copyright
Other

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