HD 65486B , the SIMBAD biblio

HD 65486B , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST15:08:25


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Title First 3 Authors
2012ApJ...755...94D 21 18 HIP 38939B: a new benchmark T dwarf in the galactic plane discovered with Pan-STARRS1. DEACON N.R., LIU M.C., MAGNIER E.A., et al.
2020A&A...633A.152C 16       D               2 62 ~ USco1621 B and USco1556 B: Two wide companions at the deuterium-burning mass limit in Upper Scorpius. CHINCHILLA P., BEJAR V.J.S., LODIEU N., et al.
2020AJ....159..257B viz 16       D               3 378 38 The Hawaii infrared parallax program. IV. A comprehensive parallax survey of L0-T8 dwarfs with UKIRT. BEST W.M.J., LIU M.C., MAGNIER E.A., et al.
2021AJ....161...42B viz 17       D               1 398 43 A volume-limited sample of ultracool dwarfs. I. Construction, space density, and a gap in the L/T transition. BEST W.M.J., LIU M.C., MAGNIER E.A., et al.
2021ApJS..253....7K viz 17       D               3 726 76 The field substellar mass function based on the full-sky 20 pc census of 525 L, T, and Y dwarfs. KIRKPATRICK J.D., GELINO C.R., FAHERTY J.K., et al.
2023A&A...670A..19G viz 17       D               1 5915 6 The Fifth Catalogue of Nearby Stars (CNS5). GOLOVIN A., REFFERT S., JUST A., et al.
2024ApJ...963...67C 18       D               2 117 ~ Predicting Cloud Conditions in Substellar Mass Objects Using Ultracool Dwarf Companions. CALAMARI E., FAHERTY J.K., VISSCHER C., et al.
2024A&A...689A.302G viz 18       D               1 1270 ~ Multiplicity of stars with planets in the solar neighbourhood. GONZALEZ-PAYO J., CABALLERO J.A., GORGAS J., et al.
2025ApJ...982...79B 112       D       C       9 106 ~ New Cold Subdwarf Discoveries from Backyard Worlds and a Metallicity Classification System for T Subdwarfs. BURGASSER A.J., SCHNEIDER A.C., MEISNER A.M., et al.
2026AJ....171..198M 20       D               4 144 ~ Uniform Forward-modeling Analysis of Ultracool Dwarfs. IV. Benchmarking the Sonora Diamondback and D. Saumon & M. S. Marley () Atmospheric Models Across Late M, L, and T Types with Low-resolution 0.8-2.5 μm Spectroscopy. MADER E., ZHANG Z., FORTNEY J.J., et al.

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