LP 119-15 , the SIMBAD biblio

LP 119-15 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST18:03:24


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Title First 3 Authors
2005AJ....129.1483L viz 63382 364 A catalog of northern stars with annual proper motions larger than 0.15" (LSPM-NORTH catalog). LEPINE S. and SHARA M.M.
2014ApJ...784..156D viz 15       D               1 1505 60 Trigonometric parallaxes for 1507 nearby mid-to-late M dwarfs. DITTMANN J.A., IRWIN J.M., CHARBONNEAU D., et al.
2016ApJ...818..153D viz 16       D               1 1874 9 Calibration of the MEarth photometric system: optical magnitudes and photometric metallicity estimates for 1802 nearby M-dwarfs. DITTMANN J.A., IRWIN J.M., CHARBONNEAU D., et al.
2016ApJ...821...93N viz 16       D               2 1898 209 The rotation and galactic kinematics of mid M dwarfs in the solar neighborhood. NEWTON E.R., IRWIN J., CHARBONNEAU D., et al.
2017ApJ...834...85N viz 16       D               1 2207 217 The Hα emission of nearby M dwarfs and its relation to stellar rotation. NEWTON E.R., IRWIN J., CHARBONNEAU D., et al.
2018AJ....155..225K viz 16       D               1 93 57 Magnetic inflation and stellar mass. II. On the radii of single, rapidly rotating, fully convective M-dwarf stars. KESSELI A.Y., MUIRHEAD P.S., MANN A.W., et al.
1995yCat.1098....0L viz 14       D               1 52096 ~ New Luyten Catalogue of stars with proper motions larger than two tenths of an arcsecond (NLTT). LUYTEN W.J.
2019ApJ...870...10M 97       D     X         3 36 8 An increased rate of large flares at intermediate rotation periods for mid-to-late M dwarfs. MONDRIK N., NEWTON E., CHARBONNEAU D., et al.
2022ApJ...927..122H viz 17       D               1 3750 2 Chemical Properties of the Local Disk and Halo. II. Abundances of 3745 M Dwarfs and Subdwarfs from Improved Model Fitting of Low-resolution Spectra. HEJAZI N., LEPINE S. and NORDLANDER T.
2025ApJ...982...98G 65       D     X         2 104 ~ Short-term Balmer Line Emission Variability in M Dwarfs. GARCIA SOTO A., DUVVURI G.M., NEWTON E.R., et al.

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