TVLM 513-42404 , the SIMBAD biblio

TVLM 513-42404 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST19:59:08


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Title First 3 Authors
1993ApJ...414..279T viz 432 72 The fainstest stars : the luminosity and mass functions at the bottom of the main sequence. TINNEY C.G.
1994AJ....108.1456R 30 18 Very low mass M dwarfs-stars or brown dwarfs in disguise? REID N., TINNEY C.G. and MOULD J.
1995AJ....110.3014T 35 79 Trigonometric parallaxes and the HR diagram at the bottom of the main sequence. TINNEY C.G., REID I.N., GIZIS J., et al.
1998A&A...337..403B viz 78 10 2358 Evolutionary models for solar metallicity low-mass stars: mass-magnitude relationships and color-magnitude diagrams. BARAFFE I., CHABRIER G., ALLARD F., et al.
1998ApJ...509..836L 97 125 Infrared colors at the stellar/substellar boundary. LEGGETT S.K., ALLARD F. and HAUSCHILDT P.H.
1998MNRAS.301.1031T viz 39 105 High-resolution spectra of very low-mass stars. TINNEY C.G. and REID I.N.
2012ApJS..201...19D viz 15       D               2 267 460 The Hawaii infrared parallax program. I. Ultracool binaries and the L/T transition. DUPUY T.J. and LIU M.C.
2017MNRAS.468.3499D viz 16       D               1 278 6 Identification of partially resolved binaries in Pan-STARRS 1 data. DEACON N.R., MAGNIER E.A., BEST W.M.J., et al.
2021A&A...649A...6G viz 17       D               1 227180 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2022A&A...660A..38W viz 17       D               1 736 1 Ultracool dwarfs identified using spectra in LAMOST DR7. WANG Y.-F., LUO A.-L., CHEN W.-P., et al.
2023AJ....165..267H viz 17       D               1 64663 1 Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., et al.
2023ApJ...959...63S 17       D               1 177 ~ The Hawaii Infrared Parallax Program. VI. The Fundamental Properties of 1000+ Ultracool Dwarfs and Planetary-mass Objects Using Optical to Mid-infrared Spectral Energy Distributions and Comparison to BT-Settl and ATMO 2020 Model Atmospheres. SANGHI A., LIU M.C., BEST W.M.J., et al.

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