Absolute magnitudes for late-type dwarf stars for Sloan photometry
Astrophysics
2009-11-10 v1
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
Cite
@article{arxiv.astro-ph/0503415,
title = {Absolute magnitudes for late-type dwarf stars for Sloan photometry},
author = {S. Bilir and S. Karaali and S. Tuncel},
journal= {arXiv preprint arXiv:astro-ph/0503415},
year = {2009}
}
Comments
11 pages, 9 figures and 5 tables, accepted for publication in AN