The low mass X-ray pulsars.

Details The low mass X-ray pulsars. The low mass X-ray pulsars.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..161m&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 161 - 162

Astronomy and Astrophysics

Astrophysics

X-Ray Pulsars: X-Ray Binaries

Scientific paper

The authors review the observational results on some peculiar X-ray pulsars with spin period in the 5-10 s range. These pulsars have many similarities, and it has been proposed that they are members of a subclass of low mass X-ray binaries (LMXBs) characterized by lower luminosities (a few 1035erg s-1), higher neutron star magnetic fields (a few 1011G), and possibly smaller ages than non-pulsating LMXBs.

Affiliated with

Also associated with

No associations

Rating

The low mass X-ray 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 The low mass X-ray pulsars., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The low mass X-ray pulsars. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-857135