Abstract
The logarithmic differential star count of the Two Micron All Sky Survey in Ks band can be well approximated by a single power-law luminosity function. With a fiducial Galactic structure, we measure the luminosity function for the entire Milky Way. The distribution of the power-law index is roughly isotropic and shows no obvious trend with the Galactic latitude. The value for the power-law index, the bright and the faint ends of the luminosity function are 1.85 ± 0.035, Ks = -7.86 ± 0.60 mag, and Ks = 6.88 ± 0.66 mag, respectively. Our result strongly supports the notion of a universal luminosity function in our Galaxy. We also find that the luminosity function of LMC/SMC is similar to that of the Milky Way.
Original language | English |
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Pages (from-to) | 182-188 |
Number of pages | 7 |
Journal | Astrophysical Journal |
Volume | 724 |
Issue number | 1 |
DOIs | |
State | Published - 20 Nov 2010 |
Keywords
- Galaxies: luminosity function, mass function
- Galaxy: fundamental parameters
- Galaxy: general
- Galaxy: stellar content
- Galaxy: structure
- Infrared: stars