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A lithium depletion boundary age of 22 Myr for NGC 1960

Jeffries, R. D.; Naylor, Tim; Mayne, N. J.; Bell, Cameron P. M.; Littlefair, S. P.

Authors

Tim Naylor

N. J. Mayne

Cameron P. M. Bell

S. P. Littlefair



Abstract

We present a deep Cousins RI photometric survey of the open cluster NGC 1960, complete to RC ≃ 22, IC ≃ 21, that is used to select a sample of very low mass cluster candidates. Gemini spectroscopy of a subset of these is used to confirm membership and locate the age-dependent ‘lithium depletion boundary’ (LDB) – the luminosity at which lithium remains unburned in its low-mass stars. The LDB implies a cluster age of 22 ± 4 Myr and is quite insensitive to choice of evolutionary model. NGC 1960 is the youngest cluster for which a LDB age has been estimated and possesses a well-populated upper main sequence and a rich low-mass pre-main sequence. The LDB age determined here agrees well with precise age estimates made for the same cluster based on isochrone fits to its high- and low-mass populations. The concordance between these three age estimation techniques, that rely on different facets of stellar astrophysics at very different masses, is an important step towards calibrating the absolute ages of young open clusters and lends confidence to ages determined using any one of them.

Citation

Jeffries, R. D., Naylor, T., Mayne, N. J., Bell, C. P. M., & Littlefair, S. P. (2013). A lithium depletion boundary age of 22 Myr for NGC 1960. Monthly Notices of the Royal Astronomical Society, 434(3), 2438-2450. https://doi.org/10.1093/mnras/stt1180

Journal Article Type Article
Acceptance Date Jun 25, 2013
Online Publication Date Aug 1, 2013
Publication Date Sep 21, 2013
Deposit Date Jun 14, 2023
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 434
Issue 3
Pages 2438-2450
DOI https://doi.org/10.1093/mnras/stt1180
Keywords Space and Planetary Science; Astronomy and Astrophysics; stars: pre-main-sequence; open clusters and associations: individual: NGC 1960