Possible observational constraints on the mass-radius relation of neutron stars

Details Possible observational constraints on the mass-radius relation of neutron stars Possible observational constraints on the mass-radius relation of neutron stars

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234..609v&link_type=abstract

Astrophysical Journal, Part 1, vol. 234, Dec. 1, 1979, p. 609-611.

Astronomy and Astrophysics

Astrophysics

55

Neutron Stars, Red Shift, Stellar Mass, X Ray Sources, Bursts, Equations Of State, Gravitational Effects, Radii

Scientific paper

The effect of gravitational redshift on the blackbody radii, as deduced
from the tails of X-ray bursts, is considered. Observed values of
blackbody radii put an upper limit to the mass and constrain the
mass-radius relations of neutron stars. Possible consequences for the
equation of state of high-density matter are briefly discussed.

Affiliated with

Also associated with

No associations

Rating

Possible observational constraints on the mass-radius relation of neutron stars 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 Possible observational constraints on the mass-radius relation of neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Possible observational constraints on the mass-radius relation of neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1442910