On the z-distribution of supernova remnants

Details On the z-distribution of supernova remnants On the z-distribution of supernova remnants

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....44...91h&link_type=abstract

Astronomy and Astrophysics, vol. 44, no. 1, Nov. 1975, p. 91-94.

Astronomy and Astrophysics

Astrophysics

10

Chemical Composition, Star Distribution, Supernova Remnants, Astronomical Models, Atomic Structure, Computerized Simulation, Mathematical Models, Radiative Recombination, Spectral Energy Distribution, Stellar Evolution, Stellar Luminosity

Scientific paper

Since observational selection effects against the detection of supernova remnants (SNR) toward high galactic latitudes cannot be ruled out, we used the existing data to determine a lower limit of detected SNR at high galactic latitudes over a significant portion of the sky and studied theoretically the dependence of the visibility of SNR on the density of the surrounding medium. These investigations lead to an improved z-distribution of SNR and show the dependence of the surface brightness on the gas density.

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