Why do collapsed stars rotate so slowly

Details Why do collapsed stars rotate so slowly Why do collapsed stars rotate so slowly

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...221..969b&link_type=abstract

Astrophysical Journal, Part 1, vol. 221, May 1, 1978, p. 969-972.

Astronomy and Astrophysics

Astrophysics

16

Gravitational Collapse, Neutron Stars, Stellar Mass Ejection, Stellar Rotation, White Dwarf Stars, Magnetic Stars, Pulsars, Stellar Evolution

Scientific paper

The case of the puzzingly slow rotation of neutron stars and white dwarfs is examined. Continuing mass loss during formation can rapidly stop the rotation of white dwarfs which have magnetic-field strengths of at least 1 million gauss, for mass-loss rates consistent with current theories. If mass loss can occur during formation of neutron stars, magnetic braking may be significant in slowing their rotation as well. The observed slow rotation of the 'nonmagnetic' white dwarfs, however, remains a mystery.

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