Journal
ASTRONOMISCHE NACHRICHTEN
Volume 326, Issue 5, Pages 321-331Publisher
WILEY-V C H VERLAG GMBH
DOI: 10.1002/asna.200510358
Keywords
techniques : Sloan photometry; stars : distances; stars : luminosity function
Categories
Ask authors/readers for more resources
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.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available