Planetary systems around radio pulsars

Details Planetary systems around radio pulsars Planetary systems around radio pulsars

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992avest..26...44t&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 26, no. 3, May-June 1992, p. 44-46. In Russian.

Astronomy and Astrophysics

Astronomy

Binary Stars, Planetary Systems, Pulsars, Radio Sources (Astronomy), Stellar Evolution, Accretion Disks, Cosmic Dust, Gravitational Collapse, Neutron Stars

Scientific paper

The paper examines possible pathways of the formation of planetary systems around radio pulsars in the course of close binary evolution. Dynamical disruption in the Roche lobe filling component leads to formation of a gas disk around a neutron star or oxygen-neon dwarf. The latter can accrete disk matter and collapse into a neutron star. The disk size increases significantly owing to viscosity; its temperature decreases, and dust particles are condensed in it. Coagulation of dust particles finally leads to accumulation of planets on circular orbits around neutron stars.

Affiliated with

Also associated with

No associations

Rating

Planetary systems around radio pulsars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Planetary systems around radio pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Planetary systems around radio pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1200791