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A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhoodAccurate parameters for HD 209458 and its planet fromHSTspectrophotometryA 0.24+0.18M_{sun}_ double-lined eclipsing binary from the HATSouth surveyThe EBLM projectThe TESS–HERMES survey data release 1: high-resolution spectroscopy of the TESS southern continuous viewing zoneKMOS view of the Galactic centre. I. Young stars are centrally concentratedBiases in the determination of dynamical parameters of star clusters: today and in the Gaia eraExamining the relationships between colour,Teff, and [M/H] for APOGEE K and M dwarfs
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Q56028360-08A26BBA-9560-4DCC-80AD-F127DE1E7E78Q56444239-09804FBB-D672-4367-A4B6-58E169FA7D6BQ56476696-C77020AE-929D-4A50-9D21-CF94ED013AE9Q56805961-24FDA9B3-30D3-417A-BFF2-D9CC22FA4503Q57442014-0A0DDBD6-95C0-469C-B382-F5A40E7D42C8Q57854094-732CEC00-4106-46FC-9EB6-DE49830937CEQ58488966-6BE18E7E-AA80-49F3-86B8-59C2CE93AF5FQ58489072-5ABD7EF2-969A-4177-9D11-68B853CD037F
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description
article
@en
im September 2014 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 2014
@uk
name
Improving PARSEC models for very low mass stars
@en
Improving PARSEC models for very low mass stars
@nl
type
label
Improving PARSEC models for very low mass stars
@en
Improving PARSEC models for very low mass stars
@nl
prefLabel
Improving PARSEC models for very low mass stars
@en
Improving PARSEC models for very low mass stars
@nl
P2093
P2860
P356
P1476
Improving PARSEC models for very low mass stars
@en
P2093
Léo Girardi
Paola Marigo
P2860
P304
P356
10.1093/MNRAS/STU1605
P407
P577
2014-09-11T00:00:00Z
P818
P819
2014MNRAS.444.2525C