Computer Science
Scientific paper
Nov 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980s%26w....19..378b&link_type=abstract
Sterne und Weltraum, vol. 19, Nov. 1980, p. 378-383. In German.
Computer Science
Neutron Stars, Stellar Radiation, Thermal Radiation, Stellar Evolution, Stellar Models, Supernovae, Surface Temperature
Scientific paper
The structure of neutron stars is examined, with emphasis on the heat content and radiated energy from the star. A schematic model is presented of the construction of a neutron star of 1.3 solar masses and the process of neutronization of material towards the center of the star is discussed. The center density, star radius, and thickness of the crust are compared according to the Reid potential method and the tensor model. Characteristics of neutron stars and black bodies are compared and the relation of neutron stars to supernovas is considered.
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