Abstract
view Abstract Citations (12) References (14) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS G 296.05-0.50 - a large diameter supernova remnant. Caswell, J. L. ; Barnes, P. L. Abstract A new map made at 408 MHz with the Molonglo Cross shows a supernova remnant (SNR) shell centered at 1 = 296.05 deg, b = -0.50 deg with a mean angular diameter of 33 arcmin. It is concluded that the X-ray emission from the region is due to a single SNR rather than two overlapping ones. As is common among SNRs, some of the stronger X-ray emission is located at a weak part of the radio shell. The distance to the object is estimated at 7.7 kpc. Other features of the map are briefly discussed. Publication: The Astrophysical Journal Pub Date: August 1983 DOI: 10.1086/184094 Bibcode: 1983ApJ...271L..55C Keywords: Radio Sources (Astronomy); Supernova Remnants; X Ray Sources; Brightness Temperature; Interstellar Gas; Light Emission; Pulsars; Astrophysics full text sources ADS | data products SIMBAD (5)
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