The origin of the planet around PSR 1829 - 10

Details The origin of the planet around PSR 1829 - 10 The origin of the planet around PSR 1829 - 10

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...382l..81n&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 382, Dec. 1, 1991, p. L81-L84. Research supported by USIBSF.

Astronomy and Astrophysics

Astrophysics

13

Companion Stars, Extrasolar Planets, Neutron Stars, Planetary Evolution, Angular Velocity, Astronomical Models, Stellar Models, Stellar Systems, Supernovae

Scientific paper

Various scenarios for formation of a planet around a neutron star, as observed in PSR 1829 - 10 are considered. It is shown that matter, ablated from a companion 1.5 solar mass star which was orbiting around the neutron star progenitor at a distance of about 3 x 10 exp 12 cm, would be captured by the neutron star and form a disk around it. The companion star escaped from the system during the supernova event, and the observed planet was eventually formed from this disk.

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