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Astrometry with Hubble Space Telescope Fine Guidance Sensors—A Review, Benedict, G. Fritz,McArthur, Barbara E.,Nelan, Edmund P., Publications of the Astronomical Society of the Pacific, 129, 2017-01-01 00:00:00, 2017PASP..129a2001B||How to Constrain Your M Dwarf. II. The Mass-Luminosity-Metallicity Relation from 0.075 to 0.70 Solar Masses, Mann, Andrew W.,Dupuy, Trent J.,Kraus, Adam L., The Astrophysical Journal, 871, 2019-01-01 00:00:00, 2019ApJ...871...63M||The Nearby Low-Mass Visual Binary Wolf 424, Torres, Guillermo,Henry, Todd J.,Franz, Otto G., The Astronomical Journal, 117, 1999-01-01 00:00:00, 1999AJ....117..562T||The Optical Mass-Luminosity Relation at the End of the Main Sequence (0.08-0.20 Msolar), Henry, Todd J.,Franz, Otto G.,Wasserman, Lawrence H., The Astrophysical Journal, 512, 1999-02-01 00:00:00, 1999ApJ...512..864H||The Solar Neighborhood. XLV. The Stellar Multiplicity Rate of M Dwarfs Within 25 pc, Winters, Jennifer G.,Henry, Todd J.,Jao, Wei-Chun, The Astronomical Journal, 157, 2019-06-01 00:00:00, 2019AJ....157..216W||The Solar Neighborhood. XXXVII: The Mass-Luminosity Relation for Main-sequence M Dwarfs, Benedict, G. F.,Henry, T. J.,Franz, O. G., The Astronomical Journal, 152, 2016-11-01 00:00:00, 2016AJ....152..141B |
