Abstract
view Abstract Citations (19) References (21) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS X-ray emission from MSH 14-63 - probable remnant of the A.D. 185 supernova. Winkler, P. F., Jr. Abstract Observations during 1972 from an experiment on OSO 7 detected a 2-10-keV X-ray flux of 1.7 by 10 to the -10th power erg/sq cm per sec from a source coincident with MSH 14-63, the most probable candidate for association with the A.D. 185 supernova. Both the present data and those of Naranan et al. (1977) at lower energy can be fitted by a dual-temperature thermal spectrum similar to that observed in other young supernova remnants. Model calculations indicate that a mass in excess of 5 solar masses must have been ejected in the A.D. 185 supernova event. Publication: The Astrophysical Journal Pub Date: April 1978 DOI: 10.1086/156020 Bibcode: 1978ApJ...221..220W Keywords: Radio Sources (Astronomy); Supernova Remnants; X Ray Astronomy; Astronomical Spectroscopy; Oso-7; Radiant Flux Density; Astrophysics; Supernova Remnants:X-Ray Sources full text sources ADS | data products SIMBAD (5)
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