X-ray halos and the size distribution of the cosmic grains

Details X-ray halos and the size distribution of the cosmic grains X-ray halos and the size distribution of the cosmic grains

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...248..624k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 2, Aug. 1991, p. 624-632.

Astronomy and Astrophysics

Astrophysics

6

Halos, Interstellar Matter, X Ray Sources, Diffraction, Heao 2, Particle Size Distribution, Refractivity

Scientific paper

Arising as a result of scattering by interstellar particles, detectable halos can surround celestial X-ray sources. The van-de-Hulst's formulation of the theory of anomalous diffraction has been used to construct intensity profiles of X-ray halos for different size distributions of the grain population. The numerical calculations demonstrate that X-ray halos could be a tracer of the size distribution of the cosmic grains.

Affiliated with

Also associated with

No associations

Rating

X-ray halos and the size distribution of the cosmic 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 X-ray halos and the size distribution of the cosmic grains, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray halos and the size distribution of the cosmic grains will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1724451