Phase-Resolved Optical Emission from Isolated Neutron Stars

Details Phase-Resolved Optical Emission from Isolated Neutron Stars Phase-Resolved Optical Emission from Isolated Neutron Stars

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999iraj...26...99s&link_type=abstract

Irish Astronomical Journal, 1999 (July), 26(2), 99

Mathematics

Logic

2

Scientific paper

In the last two years the number of pulsars with confirmed optical pulsations has increased from 3 to 5, with new `middle aged' candidate data coming to light, and several other `upper limit' objects. Based upon this growing dataset, the implications for current theoretical models for both emission theory and neutron star structure is assessed. In particular, through considerations of the resolved unpulsed predominately thermal optical flux we are able to constrain (R/d) for two nearby middle aged neutron stars, yielding upper limits for the radius of Geminga (<= 9.5 km) and the distance of PSR B0656+14 (~210 pc). From the pulsed emission we are able to show that modifications to existing phenomenological models are required to take account of emission primarily near the light cylinder.

Affiliated with

Also associated with

No associations

Rating

Phase-Resolved Optical Emission from Isolated 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 Phase-Resolved Optical Emission from Isolated Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Phase-Resolved Optical Emission from Isolated Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-995135