Absolute magnitudes for late-type dwarf stars for Sloan photometry
Preprint
- 18 March 2005
Abstract
We present a new formula for absolute magnitude determination for late-type dwarf stars as a function of (g-r) and (r-i) for Sloan photometry. The absolute magnitudes estimated by this approach are brighter than those estimated by colour-magnitude diagrams, and they reduce the luminosity function rather close to the luminosity function of Hipparcos.Keywords
All Related Versions
- Version 1, 2005-03-18, ArXiv
- Published version: Astronomische Nachrichten, 326 (5), 321.
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