XMM-Newton Timing Observations of a New X-ray Pulsar in SNR G292.0+1.8

Details XMM-Newton Timing Observations of a New X-ray Pulsar in SNR G292.0+1.8 XMM-Newton Timing Observations of a New X-ray Pulsar in SNR G292.0+1.8

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...15h&link_type=abstract

XMM-Newton Proposal ID #04003301

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Psr J1124-5916, Xmm-Newton Proposal 04003301

Scientific paper

We propose new XMM-Newton high time resolution EPIC-pn observations of a recently discovered radio and X-ray pulsar in the young oxygen-rich supernova remnant (SNR) G292.0+1.8. Our requested exposure time is sufficient to allow the first detailed study of the timing and spectral properties of the X-ray pulsar. In particular we will measure the X-ray pulse shape and phase as a function of photon energy, determine the phase lag between the radio and X-ray pulses, and measure the X-ray spectrum of the pulsed emission. Only XMM-Newton has sufficient sensitivity, high time resolution, and spectral capability to be able to study the X-ray properties of this new pulsar.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Timing Observations of a New X-ray Pulsar in SNR G292.0+1.8 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 XMM-Newton Timing Observations of a New X-ray Pulsar in SNR G292.0+1.8, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Timing Observations of a New X-ray Pulsar in SNR G292.0+1.8 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1659759