Main-Sequence Stars
Open Access
- 1 April 1959
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 119 (2) , 112-123
- https://doi.org/10.1093/mnras/119.2.112
Abstract
Integrations have been carried out for uniform stars of Types I and II. It appears likely that the separation at the zero-age main-sequence of the different populations does not exceed 0.1 magnitude, provided a correct effective temperature scale is used.Keywords
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