RICHARD Olivier n'a pas fourni de Photo.
RICHARD Olivier      
Organism : UM2
Maître de Conférences
(HDR)
Team: Astrophysique Stellaire
olivier.richard_AT_umontpellier.fr
0467144736
Room: , Floor: 4, Build.: 13

National Administration:
  • CNU
Research Topics:
  • phys/phys.astr/phys.astr.sr
  • phys/phys.astr
  • sdu/sdu.astr/sdu.astr.sr
Last scientific productions :
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+ Lithium depletion and angular momentum transport in solar-type stars doi link

Author(s): Dumont T.(Corresp.), Palacios A., Charbonnel C., Richard O., Amard L., Augustson K., Mathis S.

(Article) Published: Astronomy & Astrophysics, vol. 646 p.A48 (2021)

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+ Combining multiple structural inversions to constrain the solar modelling problem doi link

Author(s): Buldgen G., Salmon S., Noels A., Scuflaire R., Montalbán J., Baturin A., Eggenberger P., Gryaznov V., Iosilevskiy I., Meynet G., Chaplin J., Miglio A., Oreshina A., Richard O., Starostin A.

(Article) Published: Astronomy & Astrophysics, vol. 621 p.A33 (2019)
Links openAccess full text : arXiv

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. Hydrodynamical Instabilities Induced by Atomic Diffusion in F and A Stars

Author(s): Deal M., Richard O., Vauclair S.

Conference: Workshop on Astrophysical Opacities (Kalamazoo, US, 2017-08)

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. Important consequences of atomic diffusion inside main-sequence stars: opacities, extra-mixing, oscillations

Author(s): Deal M., Vauclair S., Richard O.

(Posters) Wide-Field Variability Surveys: A 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting (San Pedro de Atacama, CL), 2017

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. Hydrodynamical instabilities induced by atomic diffusion in F and A stars : Impact on the opacity profile and asteroseimic age determination

Author(s): Deal M., Richard O., Vauclair S.

Conference: SF2A-2017 (Paris, FR, 2017-07)

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