Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aj....124.2721r&link_type=abstract
The Astronomical Journal, Volume 124, Issue 5, pp. 2721-2738.
Astronomy and Astrophysics
Astronomy
129
Galaxy: Solar Neighborhood, Stars: Kinematics, Stars: Luminosity Function, Mass Function
Scientific paper
We have used new astrometric and spectroscopic observations to refine the volume-complete sample of M dwarfs defined in previous papers in this series. With the addition of Hipparcos astrometry, our revised VC2 sample includes 558 main-sequence stars in 448 systems. Analysis of that data set shows no evidence of any systematic kinematic bias. Combining those data with a Hipparcos-based sample of AFGK dwarfs within 25 pc of the Sun, we have derived the solar neighborhood luminosity function, Φ(MV), for stars with absolute magnitudes between -1 and +17. Using empirical and semiempirical mass-MV relations, we transform Φ(MV) to the present-day mass function, ψ(M) (=dN/dM). Depending on the mass-luminosity calibration adopted, ψ(M) can be represented by either a two-component or a three-component power law. In either case, the power-law index α has a value of ~1.3 at low masses (0.1 Msolar
Based partly on observations made at the 60 inch (1.5 m) telescope at Palomar Mountain, which is jointly owned by the California Institute of Technology and the Carnegie Institution of Washington.
Gizis John E.
Hawley Suzanne L.
Reid Iain Neill
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