Absolute magnitudes for late-type dwarfs (Bilir+, 2005)

Details Absolute magnitudes for late-type dwarfs (Bilir+, 2005) Absolute magnitudes for late-type dwarfs (Bilir+, 2005)

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycatp001032601b&link_type=abstract

VizieR On-line Data Catalog: J/other/AN/326.321. Originally published in: 2005AN....326..321B

Other

Stars: Late-Type, Photometry: Ugriz, Photometry: Ubvri, Photometry: Cousins, Magnitudes: Absolute

Scientific paper

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 (as defined by Abazajian et al., 2003AJ....126.2081A). 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.
(1 data file).

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