Magnetohydrodynamic model of Crab nebula radiation

Details Magnetohydrodynamic model of Crab nebula radiation Magnetohydrodynamic model of Crab nebula radiation

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...283..710k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 283, Aug. 15, 1984, p. 710-730.

Astronomy and Astrophysics

Astrophysics

305

Crab Nebula, Magnetohydrodynamics, Stellar Models, Synchrotron Radiation, Spatial Distribution, Spectral Energy Distribution

Scientific paper

The authors calculate the properties of the synchrotron continuum expected on the basis of a steady spherically symmetric MHD model of the flow in the Crab nebula. The model accounts for the spectral distribution of the continuum from the optical to γ-rays, and semiquantitatively for its observed spatial distribution. The model does not account for the radio portion of the Crab nebula's spectrum.

Affiliated with

Also associated with

No associations

Rating

Magnetohydrodynamic model of Crab nebula radiation 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 Magnetohydrodynamic model of Crab nebula radiation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetohydrodynamic model of Crab nebula radiation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1674519