binary millisecond pulsarの例文

• The "'Black Widow Pulsar "'( B1957 + 20 ) is an eclipsing binary millisecond pulsar discovered in 1988.
• Popular theories for the formation of binary millisecond pulsars require mass transfer onto the rotating neutron star from a white dwarf companion in order to spin it up to periods less than about 10 ms a process expected to be accompanied by strong tidal forces, producing a highly circular orbit.