Supernova Remnants at Meter Wavelengths (Kovalenko+ 1994)

Details Supernova Remnants at Meter Wavelengths (Kovalenko+ 1994) Supernova Remnants at Meter Wavelengths (Kovalenko+ 1994)

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..80710110k&link_type=abstract

VizieR On-line Data Catalog: J/AZh/71/110. Originally published in: 1994AZh....71..110K

Computer Science

Supernova Remnants, Radio Sources, Surveys

Scientific paper

The total flux densities of more than one hundred galactic supernova remnants (SNR) at 111, 102, and 83MHz, measured at Pushchino using the E-W WBCR-1000 and LSA radio telescopes, to an accuracy of 2Jy or better; the spectral indices, with their errors, obtained from the compiled spectra; and optical depths at 100MHz in the direction of the supernova remnants are reported. The latter values are obtained from a low frequency cutoff caused by interstellar gas absorption, which was detected at meter and decimeter wavelengths in the direction of 38% of the supernova remnants. (1 data file).

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