A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhood
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SPOTS: The Search for Planets Orbiting Two StarsCARMENES input catalogue of M dwarfsA nearby young M dwarf with a wide, possibly planetary-mass companionThe evolution of surface magnetic fields in young solar-type stars – I. The first 250 MyrOrbiting a binarySpectral and atmospheric characterization of 51 Eridani b using VLT/SPHEREThe VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbitsNear-infrared scattered light properties of the HR 4796 A dust ringCFBDSIR 2149-0403: young isolated planetary-mass object or high-metallicity low-mass brown dwarf?TheβPictoris association: Catalog of photometric rotational periods of low-mass members and candidate membersThe rotation-lithium depletion correlation in theβPictoris association and the LDB age determination
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P2860
A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhood
description
im September 2015 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 2015
@uk
name
A self-consistent, absolute is ...... ups in the solar neighbourhood
@en
A self-consistent, absolute is ...... ups in the solar neighbourhood
@nl
type
label
A self-consistent, absolute is ...... ups in the solar neighbourhood
@en
A self-consistent, absolute is ...... ups in the solar neighbourhood
@nl
prefLabel
A self-consistent, absolute is ...... ups in the solar neighbourhood
@en
A self-consistent, absolute is ...... ups in the solar neighbourhood
@nl
P2093
P2860
P356
P1476
A self-consistent, absolute is ...... ups in the solar neighbourhood
@en
P2093
Cameron P. M. Bell
Eric E. Mamajek
Tim Naylor
P2860
P304
P356
10.1093/MNRAS/STV1981
P407
P577
2015-09-24T00:00:00Z
P5875
P818
1508.05955
P819
2015MNRAS.454..593B