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Supernova remnants

Symposium - International Astronomical Union, 1967
The brightness distribution of the remnant of Tycho's Nova, which Baldwin has shown in Paper 56 (Figure 6), and the distance of 5000 pc determined by Menon and Williams (unpublished), establish beyond doubt a diameter of 10·8 pc and an average velocity of 13 300 km/sec. The initial velocity must have been higher.
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Supernovae and Their Remnants

1974
Supernovae of type II must be related to rather massive stars. They appear to occur rather exclusively in the spiral arms of galaxies and this fact alone sets a lower limit of about 5 M⊙ to their main sequence mass. If we believe that all massive stars above some critical value become supernovae (and none below this value) the supernova rate would ...
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Rectangular core-collapse supernova remnants: application to Puppis A

Monthly Notices of the Royal Astronomical Society, 2022
Alejandro Esquivel   +2 more
exaly  

New ASKAP radio supernova remnants and candidates in the Large Magellanic Cloud

Monthly Notices of the Royal Astronomical Society, 2022
Evan Crawford   +2 more
exaly  

Mixing of materials in magnetized core-collapse supernova remnants

Monthly Notices of the Royal Astronomical Society, 2023
Martin Pohl   +2 more
exaly  

Supernovae and Supernova Remnants

Annual Review of Astronomy and Astrophysics, 1964
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Supernova remnants: the X-ray perspective

Astronomy and Astrophysics Review, 2011
Jacco Vink, Vink Jacco
exaly  

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