Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Bertrand Putigny"'
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A46. ⟨10.1051/0004-6361/201935538⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A46. ⟨10.1051/0004-6361/201935538⟩
Recent numerical and theoretical considerations have shown that low-degree acoustic modes in rapidly rotating stars follow an asymptotic formula and recent observations of pulsations in rapidly rotating delta Scuti stars seem to match these expectati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e7d5f1644f82f7e3d172b8626f275e0
https://hal.archives-ouvertes.fr/hal-03101010
https://hal.archives-ouvertes.fr/hal-03101010
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 625, pp.A88. ⟨10.1051/0004-6361/201834599⟩
Astronomy and Astrophysics-A&A, 2019, 625, pp.A88. ⟨10.1051/0004-6361/201834599⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 625, pp.A88. ⟨10.1051/0004-6361/201834599⟩
Astronomy and Astrophysics-A&A, 2019, 625, pp.A88. ⟨10.1051/0004-6361/201834599⟩
The understanding of the evolution of early-type stars is tightly related to that of the effects of rapid rotation. For massive stars, rapid rotation combines with their strong radiation-driven wind. The aim of this paper is to investigate two questi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::143569e606140ab033f993be1fd9830f
https://hal.archives-ouvertes.fr/hal-02918690/document
https://hal.archives-ouvertes.fr/hal-02918690/document
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 625, pp.A89. ⟨10.1051/0004-6361/201832581⟩
Astronomy and Astrophysics-A&A, 2019, 625, pp.A89. ⟨10.1051/0004-6361/201832581⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 625, pp.A89. ⟨10.1051/0004-6361/201832581⟩
Astronomy and Astrophysics-A&A, 2019, 625, pp.A89. ⟨10.1051/0004-6361/201832581⟩
The understanding of the rotational evolution of early-type stars is deeply related to that of anisotropic mass and angular momentum loss. In this paper, we aim to clarify the rotational evolution of rapidly rotating early-type stars along the main s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f09fbe9b1634a252652365238749907
https://hal.archives-ouvertes.fr/hal-02918686
https://hal.archives-ouvertes.fr/hal-02918686
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 619, pp.A167. ⟨10.1051/0004-6361/201833450⟩
Astronomy and Astrophysics-A&A, 2018, 619, pp.A167. ⟨10.1051/0004-6361/201833450⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 619, pp.A167. ⟨10.1051/0004-6361/201833450⟩
Astronomy and Astrophysics-A&A, 2018, 619, pp.A167. ⟨10.1051/0004-6361/201833450⟩
Gravity darkening (GD) and flattening are important consequences of stellar rotation. The precise characterization of these effects across the HRD is crucial to a deeper understanding of stellar structure and evolution. We seek to characterize such i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e0883af7ee51e6d9a85360f8b7adfe5
Stars may be understood as self-gravitating masses of a compressible fluid whose radiative cooling is compensated by nuclear reactions or gravitational contraction. The understanding of their time evolution requires the use of detailed models that ac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2dada168ec701465e8b5e99119ed9386
http://arxiv.org/abs/1605.02359
http://arxiv.org/abs/1605.02359
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 609 (A124), ⟨10.1051/0004-6361/201731729⟩
Astronomy and Astrophysics-A&A, 2018, 609 (A124), ⟨10.1051/0004-6361/201731729⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 609 (A124), ⟨10.1051/0004-6361/201731729⟩
Astronomy and Astrophysics-A&A, 2018, 609 (A124), ⟨10.1051/0004-6361/201731729⟩
Recent interferometric data have been used to constrain the brightness distribution at the surface of nearby stars, in particular the so-called gravity darkening that makes fast rotating stars brighter at their poles than at their equator. However, g
Publikováno v:
HPCS
International Conference on High Performance Computing & Simulation (HPCS 2014)
International Conference on High Performance Computing & Simulation (HPCS 2014), Jul 2014, Bologna, Italy. ⟨10.1109/HPCSim.2014.6903790⟩
International Conference on High Performance Computing & Simulation (HPCS 2014)
International Conference on High Performance Computing & Simulation (HPCS 2014), Jul 2014, Bologna, Italy. ⟨10.1109/HPCSim.2014.6903790⟩
International audience; The increasing computation capability of servers comes with a dramatic increase of their complexity through many cores, multiple levels of caches and NUMA architectures. Exploiting the computing power is increasingly harder an
Publikováno v:
IPDPS Workshops
PDSEC-The 15th IEEE International Workshop on Parallel and Distributed Scientific and Engineering Computing, held in conjunction with IPDPS
PDSEC-The 15th IEEE International Workshop on Parallel and Distributed Scientific and Engineering Computing, held in conjunction with IPDPS, May 2014, Phoenix, AZ, United States. ⟨10.1109/IPDPSW.2014.139⟩
PDSEC-The 15th IEEE International Workshop on Parallel and Distributed Scientific and Engineering Computing, held in conjunction with IPDPS
PDSEC-The 15th IEEE International Workshop on Parallel and Distributed Scientific and Engineering Computing, held in conjunction with IPDPS, May 2014, Phoenix, AZ, United States. ⟨10.1109/IPDPSW.2014.139⟩
International audience; Shared memory MPI communication is an important part of the overall performance of parallel applications. However understanding the behavior of these data transfers is difficult because of the combined complexity of modern mem