Accretion onto neutron stars with the presence of a double layer

Details Accretion onto neutron stars with the presence of a double layer Accretion onto neutron stars with the presence of a double layer

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...305..759w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 305, June 15, 1986, p. 759-766.

Astronomy and Astrophysics

Astrophysics

11

Neutron Stars, Plasma Layers, Pulsars, Stellar Mass Accretion, X Ray Binaries, Electron Density (Concentration), Kinetic Energy, Poisson Equation, Vlasov Equations

Scientific paper

It is known from laboratory experiments that double layers can form in plasmas, usually in the presence of an electric current. It is argued that a double layer may be present in the accretion column of a neutron star in a binary system. It is suggested that the double layer may be the predominant deceleration mechanism for the accreting ions, especially for sources with X-ray luminosities of less than about 10 to the 37th erg/s. Previous models have involved either a collisionless shock or an assumed gradual deceleration of the accreting ions to thermalize the energy of the infalling matter.

Affiliated with

Also associated with

No associations

Rating

Accretion onto neutron stars with the presence of a double layer 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 Accretion onto neutron stars with the presence of a double layer, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Accretion onto neutron stars with the presence of a double layer will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1830286