Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phdt.........1b&link_type=abstract
Thesis Max-Planck-Inst. für Physik und Astrophysik, Garching (Germany, F.R.). Inst. für Extraterrestrische Physik.
Astronomy and Astrophysics
Astronomy
7
Computerized Simulation, Crab Nebula, Interactions, Pulsars, X Ray Astronomy, Heao 2, High Resolution, Satellite Imagery, Synchrotron Radiation, X Ray Spectra
Scientific paper
The measured soft x ray brightness of Crab nebula and simulated data are compared. The aim is a better understanding of the conversion of the Crab pulsar's rotational energy into synchrotron radiation. The soft x ray data obtained in 1979 by the high resolution imager on the Einstein observatory is compared with the brightness distribution of a three dimensional model, based on theoretical concepts developed by Rees and Gunn in 1974 and by Aschenbach and Brinkmann in 1975.
No associations
LandOfFree
On the interaction of a pulsar with the ambient medium utilizing X ray images of the Crab nebula 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 On the interaction of a pulsar with the ambient medium utilizing X ray images of the Crab nebula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the interaction of a pulsar with the ambient medium utilizing X ray images of the Crab nebula will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1520979