Mass-to-Radius Ratio Measurement of the Millisecond Pulsar J0030+0451

Details Mass-to-Radius Ratio Measurement of the Millisecond Pulsar J0030+0451 Mass-to-Radius Ratio Measurement of the Millisecond Pulsar J0030+0451

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop...86b&link_type=abstract

XMM-Newton Proposal ID #05022901

Other

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Psr J0030+0451, Xmm-Newton Proposal 05022901

Scientific paper

Modeling the thermal X-ray spectra and pulse profiles of radio millisecond pulsars (MSPs) provides important insight into the properties of neutron stars (NSs). In the nearest MSP, J0437--4715, with such modeling we are able to place constraints on the mass-to-radius ratio of the star, the B-field geometry, and surface properties. Application of this powerful method on another system would provide a crucial validity check and allow an additional set of measuremens. An XMM-Newton X-ray study of the nearby PSR J0030+0451, may lead to a major advance towards constraining the NS equation of state and other important NS parameters.

Affiliated with

Also associated with

No associations

Rating

Mass-to-Radius Ratio Measurement of the Millisecond Pulsar J0030+0451 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 Mass-to-Radius Ratio Measurement of the Millisecond Pulsar J0030+0451, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass-to-Radius Ratio Measurement of the Millisecond Pulsar J0030+0451 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1022551