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Supernovae and the Ap Phenomenon

Published online by Cambridge University Press:  14 August 2015

R. Rajamohan  and
Ashok K. Pati
R. Rajamohan
Affiliation:
Indian Institute of Astrophysics, Bangalore-560 034, India
Ashok K. Pati
Affiliation:
Indian Institute of Astrophysics, Bangalore-560 034, India

Extract

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We present evidence that relates the phenomenon of the chemically peculiar stars of the upper main sequence to supernovae explosions in young galactic clusters and associations. In the Upper Scorpius region of the Scorpio-Centaurus association we find that the radio shell discovered by Sancisi and Van Woerden (1970) from 21 cm observations and interpreted by them as an old supernova remnant has interacted with dense clouds. This remnant is seen clearly in the deep sky, narrow-band, H-alpha pictures of Sivan (1974). We find that the peculiar stars lie close to, or along the edges of, the interaction.

Type
August 28 Open Clusters
Information
Symposium - International Astronomical Union , Volume 85: Star Clusters , 1980 , pp. 251
Copyright
Copyright © Reidel 1980 

References

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