The Enigmatic Compact Object in the Stellar System LS I +61°303: Accreting or Not Accreting?

Details The Enigmatic Compact Object in the Stellar System LS I +61°303: Accreting or Not Accreting? The Enigmatic Compact Object in the Stellar System LS I +61°303: Accreting or Not Accreting?

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..924..729m&link_type=abstract

THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS. AIP Conference Proceedings, Volume 924, pp. 729-736

Computer Science

2

X-Ray Binaries, Accretion And Accretion Disks, Gamma-Ray Sources, Gamma-Ray Bursts, Radio Sources

Scientific paper

LS I +61°303 is up to now the only X-ray binary stellar system
having variable TeV gamma-ray emission and periodic radio-outbursts that
have been spatially resolved in ejecta with different position angles at
the different epochs. We review here the data and discuss the two
alternative models: a precessing microblazar or a young pulsar.

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