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- W2596257601 abstract "We report on new measurements of the luminosity function (LF) and mass function (MF) of field low-mass dwarfs derived from Sloan Digital Sky Survey Data Release 6 photometry. The analysis incorporates ∼15 million low-mass stars (0.1 M� < M < 0.8 M� ), spread over 8400 deg 2 . Stellar distances are estimated using new photometric parallax relations, constructed from ugriz photometry of nearby low-mass stars with trigonometric parallaxes. We use a technique that simultaneously measures Galactic structure and the stellar LF from 7 <M r < 16. We compare the LF to previous studies and convert to an MF using the mass–luminosity relations of Delfosse et al. The system MF, measured over −1.0 < log M/M� < −0.1, is well described by a lognormal distribution with M◦ = 0.25 M� . We stress that our results should not be extrapolated to other mass regimes. Our work generally agrees with prior low-mass stellar MFs and places strong constraints on future theoretical star formation studies." @default.
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- W2596257601 date "2010-04-22" @default.
- W2596257601 modified "2023-10-16" @default.
- W2596257601 title "THE LUMINOSITY AND MASS FUNCTIONS OF LOW-MASS STARS IN THE GALACTIC DISK. II. THE FIELD" @default.
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