Supernova Remnants at Meter Wavelengths : J/AZh/71/110

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Authors : Kovalenko A.V. orcid , Pynzar A.V., Udaltsov V.A. (hide) , Pynzar A.V., Udaltsov V.A. et..al

VizieR DOI :
Bibcode : 1994AZh....71..110K (ADS) (Simbad) (Objects)
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CDS Keywords : Supernova remnants; Radio sources; Surveys
UAT : Supernova remnants, Radio sources, Surveys

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Inserted into VizieR : 14-Oct-1997
Last modification : 09-Dec-1997

Observations of Supernova Remnants at Pushchino Catalog of Flux Densities at Meter Wavelengths. (1994)

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Abstract: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. ...(more)
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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. 


                


                

                    

                


                

                    

                


                

                    
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