Origin of millisecond pulsars

Details Origin of millisecond pulsars Origin of millisecond pulsars

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987natur.329..310m&link_type=abstract

Nature, Volume 329, Issue 6137, pp. 310-312 (1987).

Physics

64

Scientific paper

The recent discovery1,2 of a 3-millisecond pulsar in the globular cluster M28 (NGC6626) suggests that a few per cent of type I super novae (of which there are several subcategories, all associated with old stellar populations) form neutron stars. If the contact-binary white dwarf model for type Is is invoked3, it seems probable that millisecond pulsars of low magnetic field would be formed in binary systems which might survive the supernova event.

Affiliated with

Also associated with

No associations

Rating

Origin of millisecond 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 Origin of millisecond pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Origin of millisecond pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1676818