Accretion induced collapse and field decay

Details Accretion induced collapse and field decay Accretion induced collapse and field decay

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..677w&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 677-681 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

Magnetic Field Configurations, Pulsars, Star Formation, Stellar Magnetic Fields, Stellar Mass Accretion, Gravitational Collapse, Gravitational Effects, Neutron Stars, Stellar Gravitation, Stellar Models, White Dwarf Stars, X Ray Astronomy

Scientific paper

The suggestion that neutron stars can be formed via accretion-induced collapse of a white dwarf is considered. It is shown that this suggestion is not viable for 4U1626-67 and Her X-1. This leads to the suggestion that some neutron stars may grow old without losing their strong magnetic fields. It implies that there is no observational evidence for the occurrence of accretion-induced collapse in any of the systems for which this process was hitherto suggested.

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