On Super-novae
- Creators
- Baade, W.
- Zwicky, F.
Abstract
The extensive investigations of extragalactic systems during recent years have brought to light the remarkable fact that there exist two well-defined types of new stars or novae which might be distinguished as common novae and super-novae. No intermediate objects have so far been observed. Common novae seem to be a rather frequent phenomenon in certain stellar systems. Thus, according to Bailey [1], ten to twenty novae flash up every year in our own Milky Way. A similar frequency (30 per year) has been found by Hubble in the well-known Andromeda nebula. A characteristic feature of these common novae is their absolute brightness (M) at maximum, which in the mean is -5.8 with a range of perhaps 3 to 4 mags. The maximum corresponds to 20,000 times the radiation of the sun. During maximum light the common novae therefore belong to the absolutely brightest stars in stellar systems. This is in full agreement with the fact that we have been able to discover this type of novae in other stellar systems near enough for us to reach stars of absolute magnitude -5 with our present optical equipment.
Additional Information
Copyright © 1934 by the National Academy of Sciences Communicated March 19, 1934Files
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Additional details
- Eprint ID
- 6942
- Resolver ID
- CaltechAUTHORS:BAApnas34a
- Created
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2007-01-03Created from EPrint's datestamp field
- Updated
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2019-10-02Created from EPrint's last_modified field