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The Metallic Hydride Dwarfs

Published online by Cambridge University Press:  25 April 2016

M.S. Bessell
M.S. Bessell*
Affiliation:
Mount Stromlo and Siding Spring Observatories, A.N.U.
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Extract

The properties of the M dwarfs have been investigated by spectroscopic and photometric observations of over 150 red, high proper motion stars. Most of these stars have red magnitudes fainter than 12 magnitude.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 4 , 1982 , pp. 417 - 419
Copyright
Copyright © Astronomical Society of Australia 1982

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References

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