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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Nova, which Baldwin has shown in Paper 56 (Figure 6), and the distance of 5000 pc determined by Menon and Williams (unpublished), establish beyond doubt a diameter of 10·8 pc and an average velocity of 13 300 km/sec.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.
openaire   +1 more source

Supernovae and supernova remnants

1974
C. B. Cosmovici   +2 more
openaire   +3 more sources

The infancy of core-collapse supernova remnants

Monthly Notices of the Royal Astronomical Society, 2021
Annop Wongwathanarat   +2 more
exaly  

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 ...
openaire   +1 more source

Morphology of supernova remnants and their halos

Astronomy and Astrophysics, 2021
Martin Pohl   +2 more
exaly  

Non-thermal radio supernova remnants of exiled Wolf–Rayet stars

Monthly Notices of the Royal Astronomical Society, 2021
Martin Pohl, Dominique M -A Meyer
exaly  

Cosmic ray electrons released by supernova remnants

Monthly Notices of the Royal Astronomical Society, 2021
Giovanni Morlino, Silvia Celli
exaly  

Supernovae and Supernova Remnants

Annual Review of Astronomy and Astrophysics, 1964
openaire   +1 more source

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