Zobrazeno 1 - 10
of 116
pro vyhledávání: '"T. Constantino"'
Autor:
I, Baraffe, T, Constantino, J, Clarke, A, Le Saux, T, Goffrey, T, Guillet, J, Pratt, G, Vlaykov D.
Publikováno v:
A&A 659, A53 (2022)
Recent hydrodynamical simulations of convection in a solar-like model suggest that penetrative convective flows at the boundary of the convective envelope modify the thermal background in the overshooting layer. Based on these results, we implement i
Externí odkaz:
http://arxiv.org/abs/2201.00200
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 514:715-727
Stellar convection is a non-local process responsible for the transport of heat and chemical species. It can lead to enhanced mixing through convective overshooting and excitation of internal gravity waves (IGWs) at convective boundaries. The relatio
Autor:
I Baraffe, J Clarke, A Morison, D G Vlaykov, T Constantino, T Goffrey, T Guillet, A Le Saux, J Pratt
We perform two-dimensional numerical simulations of core convection for zero-age-main-sequence stars covering a mass range from 3 $M_\odot$ to 20 $M_\odot$. The simulations are performed with the fully compressible time-implicit code MUSIC. We study
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6703d4aac56b2ec418a870917af871de
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2023, 522 (2), pp.2835-2849. ⟨10.1093/mnras/stad1067⟩
Mon.Not.Roy.Astron.Soc., 2023, 522 (2), pp.2835-2849. ⟨10.1093/mnras/stad1067⟩
Main-sequence intermediate-mass stars present a radiative envelope that supports internal gravity waves (IGWs). Excited at the boundary with the convective core, IGWs propagate towards the stellar surface and are suspected to impact physical processe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64fad15fd2efbab00b97afbf94f96c1b
https://hal.science/hal-04084071
https://hal.science/hal-04084071
Publikováno v:
Journal of Clinical and Laboratory Research. 3:01-15
Dengue virus is the most common mosquito borne viral disease in humans, and poses a major challenge to global public health services. Infection can be caused by any of the 4 DENV serotypes, transmitted by female Aedes aegypti mosquitoes. Presenting f
Autor:
A. Le Saux, T. Guillet, I. Baraffe, D. G. Vlaykov, T. Constantino, J. Pratt, T. Goffrey, M. Sylvain, V. Réville, A. S. Brun
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 660, ⟨10.1051/0004-6361/202142569⟩
Astronomy and Astrophysics-A&A, 2022, 660, ⟨10.1051/0004-6361/202142569⟩
Artificially increasing the luminosity and the thermal diffusivity of a model is a common tactic adopted in hydrodynamical simulations of stellar convection. In this work, we analyse the impact of these artificial modifications on the physical proper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4abac7702460a26ece3b90e347776afa
https://hal-insu.archives-ouvertes.fr/insu-03672033/file/aa42569-21.pdf
https://hal-insu.archives-ouvertes.fr/insu-03672033/file/aa42569-21.pdf
Autor:
T. Constantino, D. G. Vlaykov, Isabelle Baraffe, Jane Pratt, A. Le Saux, T. Goffrey, T. Guillet
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 654, ⟨10.1051/0004-6361/202140441⟩
Astronomy and Astrophysics-A&A, 2021, 654, ⟨10.1051/0004-6361/202140441⟩
We perform 2D, fully compressible, time-implicit simulations of convection in a solar-like model with the MUSIC code. Our main motivation is to explore the impact of a common tactic adopted in numerical simulations of convection that use realistic st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f005b16b358d076140f7dacd86ec57d7
http://arxiv.org/abs/2109.00943
http://arxiv.org/abs/2109.00943
Publikováno v:
Laboratory Medicine. 50:e82-e90
Nucleated red blood cells (RBCs) are normally observed in the peripheral blood of neonates and during pregnancy. Under other conditions, the presence of nucleated RBCs in circulating blood indicates disorder in the blood-producing mechanism. The incr
Publikováno v:
Astronomy & Astrophysics
Autor:
Maurizio Salaris, V. Silva Aguirre, Santi Cassisi, Anwesh Mazumdar, Dennis Stello, George C. Angelou, Andrea Miglio, R. M. Ouazzani, Federico Spada, Earl P. Bellinger, Diego Bossini, Tiara Battich, M. M. Miller Bertolami, Jakob Rørsted Mosumgaard, Richard H. D. Townsend, K. B. Nielsen, Adriano Pietrinferni, Chen Jiang, S. Deheuvels, Saskia Hekker, A. Weiss, Jørgen Christensen-Dalsgaard, Aldo Serenelli, T. Constantino, Patrick Eggenberger, Yveline Lebreton
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Silva Aguirre, V, Christensen-Dalsgaard, J, Cassisi, S, Miller Bertolami, M, Serenelli, A, Stello, D, Weiss, A, Angelou, G, Jiang, C, Lebreton, Y, Spada, F, Bellinger, E P, Deheuvels, S, Ouazzani, R M, Pietrinferni, A, Mosumgaard, J R, Townsend, R H D, Battich, T, Bossini, D, Constantino, T, Eggenberger, P, Hekker, S, Mazumdar, A, Miglio, A, Nielsen, K B & Salaris, M 2020, ' The Aarhus red giants challenge. I. Stellar structures in the red giant branch phase ', Astronomy & Astrophysics, vol. 635, A164 . https://doi.org/10.1051/0004-6361/201935843
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and Astrophysics-A&A, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Silva Aguirre, V, Christensen-Dalsgaard, J, Cassisi, S, Miller Bertolami, M, Serenelli, A, Stello, D, Weiss, A, Angelou, G, Jiang, C, Lebreton, Y, Spada, F, Bellinger, E P, Deheuvels, S, Ouazzani, R M, Pietrinferni, A, Mosumgaard, J R, Townsend, R H D, Battich, T, Bossini, D, Constantino, T, Eggenberger, P, Hekker, S, Mazumdar, A, Miglio, A, Nielsen, K B & Salaris, M 2020, ' The Aarhus red giants challenge. I. Stellar structures in the red giant branch phase ', Astronomy & Astrophysics, vol. 635, A164 . https://doi.org/10.1051/0004-6361/201935843
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
[Context] With the advent of space-based asteroseismology, determining accurate properties of red-giant stars using their observed oscillations has become the focus of many investigations due to their implications in a variety of fields in astrophysi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32ca00bc11201ce0701dca512053533b
https://hal.science/hal-02523040/file/aa35843-19.pdf
https://hal.science/hal-02523040/file/aa35843-19.pdf