Parallaxes of Southern Extremely Cool objects III: 118 L and T dwarfs

Autor: Mariateresa Crosta, Alexandre Humberto Andrei, J. L. Penna, D. N. da Silva Neto, D. J. Pinfield, Alessandro Sozzetti, Federico Marocco, Rene A. Mendez, M. Daprà, Alberto Vecchiato, R. Lachaume, Massimiliano Lattanzi, Julio Camargo, James S. Jenkins, Ben Burningham, Richard L. Smart, Beatrice Bucciarelli, V. A. d'Ávila, Bertrand Goldman, Hugh R. A. Jones
Přispěvatelé: ITA, USA, GBR, DEU, BRA, CHL, LaserLaB - Physics of Light, Atoms, Molecules, Lasers
Rok vydání: 2018
Předmět:
Zdroj: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 481(3), 3548-3562. Oxford University Press
Smart, R L, Bucciarelli, B, Jones, H R A, Marocco, F, Andrei, A H, Goldman, B, Mendez, R A, d'Avila, V A, Burningham, B, Camargo, J I B, Crosta, M T, Daprà, M, Jenkins, J S, Lachaume, R, Lattanzi, M G, Penna, J L, Pinfield, D J, da Silva Neto, D N, Sozzetti, A & Vecchiato, A 2018, ' Parallaxes of Southern Extremely Cool objects III : 118 L and T dwarfs ', Monthly Notices of the Royal Astronomical Society, vol. 481, no. 3, pp. 3548-3562 . https://doi.org/10.1093/mnras/sty2520
ISSN: 1365-2966
0035-8711
DOI: 10.1093/mnras/sty2520
Popis: We present new results from the Parallaxes of Southern Extremely Cool dwarfs program to measure parallaxes, proper motions and multi-epoch photometry of L and early T dwarfs. The observations were made on 108 nights over the course of 8 years using the Wide Field Imager on the ESO 2.2m telescope. We present 118 new parallaxes of L \& T dwarfs of which 52 have no published values and 24 of the 66 published values are preliminary estimates from this program. The parallax precision varies from 1.0 to 15.5 mas with a median of 3.8 mas. We find evidence for 2 objects with long term photometric variation and 24 new moving group candidates. We cross-match our sample to published photometric catalogues and find standard magnitudes in up to 16 pass-bands from which we build spectral energy distributions and H-R diagrams. This allows us to confirm the theoretically anticipated minimum in radius between stars and brown dwarfs across the hydrogen burning minimum mass. We find the minimum occurs between L2 and L6 and verify the predicted steep dependence of radius in the hydrogen burning regime and the gentle rise into the degenerate brown dwarf regime. We find a relatively young age of 2 Gyr from the kinematics of our sample.
Comment: In press MNRAS
Databáze: OpenAIRE