4.7 Article

A lithium depletion boundary age of 21 Myr for the Beta Pictoris moving group

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnrasl/slt141

关键词

stars: kinematics and dynamics; stars: late-type; stars: pre-main sequence; open clusters and associations: individual: Beta Pictoris; solar neighbourhood

资金

  1. European Union [312430]
  2. STFC
  3. STFC [ST/J000035/1, ST/G002355/1, ST/I005749/1, ST/J001384/1, PP/D000955/1, PP/F000057/1] Funding Source: UKRI
  4. Science and Technology Facilities Council [PP/F000057/1, ST/G002355/1, ST/J000035/1, ST/I005749/1, PP/D000955/1, ST/J001384/1] Funding Source: researchfish

向作者/读者索取更多资源

Optical spectroscopy is used to confirm membership for eight low-mass candidates in the young Beta Pic moving group (BPMG) via their radial velocities, chromospheric activity and kinematic parallaxes. We searched for the presence of the Li I 6708 angstrom resonance feature and combined the results with literature measurements of other BPMG members to find the age-dependent lithium depletion boundary (LDB) - the luminosity at which Li remains unburned in a coeval group. The LDB age of the BPMG is 21 +/- 4 Myr and insensitive to the choice of low-mass evolutionary models. This age is more precise, likely to be more accurate, and much older than that commonly assumed for the BPMG. As a result, substellar and planetary companions of BPMG members will be more massive than previously thought.

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