activity
19982022
most citedA probable stellar solution to the cosmological lithium discrepancy

322 citations · 1.6k across the 32 of their papers we have counts for

collaborators

32 papers

astro-ph.SR2022★ 7 cited

Analysis of eight magnetic chemically peculiar stars with rotational modulation

O. Kobzar, V. Khalack, D. Bohlender +9

Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) has provided stellar photometry to the astronomical community. We have used TESS data to study rotational mo…

astro-ph.SR2022★ 29 cited

Discovery of a thin lithium plateau among metal-poor red giant branch stars

A. Mucciarelli, L. Monaco, P. Bonifacio +5

The surface lithium abundance A(Li) of warm metal-poor dwarf stars exhibits a narrow plateau down to [Fe/H]~-2.8 dex, while at lower metallicities the average value drops by 0.3 de…

astro-ph.SR2021★ 6 cited

New nickel opacities and their impact on stellar models

A. Hui-Bon-Hoa, J. -C. Pain, O. Richard

The chemical element nickel is of particular interest in stellar physics. In the layers in which the Fe-peak elements dominate the mean opacity (the so-called Z-bump), Ni is the se…

astro-ph.SR2021★ 12 cited

Matter accretion in metal-poor stars down to extremely metal-poor stars and the lithium problem

M. Deal, O. Richard, S. Vauclair

The formation and evolution of light elements in the Universe act as important cosmological constraints. It has long been assumed that the oldest stars of the Galaxy display the pr…

astro-ph.SR2020★ 49 cited

Lithium depletion and angular momentum transport in solar-type stars

T. Dumont, A. Palacios, C. Charbonnel +4

Transport processes occurring in the radiative interior of solar-type stars are evidenced by the surface variation of light elements, in particular Li, and the evolution of their r…

astro-ph.SR2020★ 1 cited

Study of slowly rotating CP stars observed with TESS

O. Kobzar, V. Khalack, D. Bohlender +10

Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) provides high-quality space data on stellar photometry to the astronomical community. We present the results…