The X-ray pulsed fraction of NP0532 and interstellar grains

Details The X-ray pulsed fraction of NP0532 and interstellar grains The X-ray pulsed fraction of NP0532 and interstellar grains

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasau...2..325t&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 9th, Parkes, New South Wales, Australia, May 14-16, 1975.) Astronomi

Astronomy and Astrophysics

Astronomy

1

Cosmic Dust, Crab Nebula, Interstellar Matter, Pulsars, X Ray Astronomy, Astronomical Models, Astronomical Spectroscopy, Line Shape, Stellar Spectra, X Ray Scattering, X Ray Stars

Scientific paper

According to the currently available data on the measured pulsed fraction of X-rays from the Crab Nebula between the energies 0.7 and 300 keV, it is no longer necessary to postulate on intrinsic change in the pulsar spectral index near 30 keV. The spectral flattening which is evident at low energies can be entirely attributed to the destruction of time coherence of the pulse structure by the scattering action of interstellar dust grains.

Affiliated with

Also associated with

No associations

Rating

The X-ray pulsed fraction of NP0532 and interstellar grains 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 X-ray pulsed fraction of NP0532 and interstellar grains, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The X-ray pulsed fraction of NP0532 and interstellar grains will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1746952