Spectroscopic Survey of M Dwarfs within 100 Parsecs of the Sun
- 1 October 2005
- journal article
- Published by American Astronomical Society in The Astronomical Journal
- Vol. 130 (4) , 1871-1879
- https://doi.org/10.1086/444417
Abstract
No abstract availableKeywords
This publication has 22 references indexed in Scilit:
- The Sun's Distance from the Galactic PlaneAstrophysics and Space Science, 2003
- Revised Coordinates and Proper Motions of the Stars in the Luyten Half‐Second CatalogThe Astrophysical Journal Supplement Series, 2002
- The Palomar/MSU Nearby Star Spectroscopic Survey. III. Chromospheric Activity, M Dwarf Ages, and the Local Star Formation HistoryThe Astronomical Journal, 2002
- M-Subdwarfs: Spectroscopic Classification and the Metallicity ScaleThe Astronomical Journal, 1997
- The Palomar/MSU Nearby Star Spectroscopic Survey.II.The Southern M Dwarfs and Investigation of Magnetic ActivityThe Astronomical Journal, 1996
- The luminosity function at the end of the main sequence: Results of a deep, large-area, CCD survey for cool dwarfsThe Astrophysical Journal Supplement Series, 1994
- M dwarf spectra from 0.6 to 1.5 micron - A spectral sequence, model atmosphere fitting, and the temperature scaleThe Astrophysical Journal, 1993
- Infrared colors of low-mass starsThe Astrophysical Journal Supplement Series, 1992
- Heating of galactic discs with realistic vertical potentialsMonthly Notices of the Royal Astronomical Society, 1992
- Calculating galactic space velocities and their uncertainties, with an application to the Ursa Major groupThe Astronomical Journal, 1987