Zobrazeno 1 - 10
of 142
pro vyhledávání: '"T. van Reeth"'
Publikováno v:
BioTechniques, Vol 25, Iss 5, Pp 898-904 (1998)
Epitope tagging simplifies detection, characterization and purification of proteins. Gene fusion to combine the coding region of a well-characterized epitope with the coding region for a protein of interest generally requires several subcloning steps
Externí odkaz:
https://doaj.org/article/b499bd87e15247bebfbd57695d51a7ea
Akademický článek
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Akademický článek
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Publikováno v:
Astronomy & Astrophysics, 670, pp. 1-13
Astronomy & Astrophysics, 670, 1-13
Astronomy & Astrophysics, 670, 1-13
Context. Unambiguous examples of the influence of tides on self-excited, free stellar pulsations have recently been observationally detected in space-based photometric data. Aims. We aim to investigate U Gru and contextualise it within the growing cl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d32bea3cddb4f4e4fafa4efd1e296bb
http://arxiv.org/abs/2210.06491
http://arxiv.org/abs/2210.06491
Autor:
J A Toalá, D M Bowman, T Van Reeth, H Todt, K Dsilva, T Shenar, G Koenigsberger, S Estrada-Dorado, L M Oskinova, W-R Hamann
We present the analysis of the optical variability of the early, nitrogen-rich Wolf-Rayet (WR) star WR7. The analysis of multi-sector Transiting Exoplanet Survey Satellite (TESS) light curves and high-resolution spectroscopic observations confirm mul
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0781e4fc7af3438f0cc45b2b071a5bdc
https://lirias.kuleuven.be/handle/20.500.12942/700308
https://lirias.kuleuven.be/handle/20.500.12942/700308
Autor:
T. Van Reeth, P. De Cat, J. Van Beeck, V. Prat, D. J. Wright, H. Lehmann, A.-N. Chené, E. Kambe, S. L. S. Yang, G. Gentile, M. Joos
The TESS space mission provides us with high-precision photometric observations of bright stars over more than 70% of the entire sky, allowing us to revisit and characterise well-known stars. We aim to conduct an asteroseismic analysis of the gamma D
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::166e7d459a82271df4959a4d2bca8afc
https://resolver.caltech.edu/CaltechAUTHORS:20220614-222204000
https://resolver.caltech.edu/CaltechAUTHORS:20220614-222204000
Akademický článek
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Publikováno v:
Astronomy & Astrophysics, 662, pp. 1-15
Astronomy & Astrophysics, 662, 1-15
Astronomy & Astrophysics, 662, 1-15
Context: the theory of stellar evolution presents shortcomings when confronted with asteroseismic probes of interior physical properties. The differences between observations and theory are often great because stellar models have mainly been calibrat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a6a3753fc5169b1a4f778378b390fcca
https://doi.org/10.1051/0004-6361/202141926
https://doi.org/10.1051/0004-6361/202141926
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 661, pp.A133. ⟨10.1051/0004-6361/202142956⟩
Astronomy & Astrophysics, 661, 1-21
Astronomy & Astrophysics, 661, pp. 1-21
Astronomy and Astrophysics-A&A, 2022, 661, pp.A133. ⟨10.1051/0004-6361/202142956⟩
Astronomy & Astrophysics, 661, 1-21
Astronomy & Astrophysics, 661, pp. 1-21
Asteroseismology has revealed small core-to-surface rotation contrasts in stars in the whole HR diagram. This is the signature of strong transport of angular momentum (AM) in stellar interiors. One of the plausible candidates to efficiently carry AM
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4051aa442dff1e1fc0eb8749f9f82312
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 656, pp.A122. ⟨10.1051/0004-6361/202141152⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 656, pp.A122. ⟨10.1051/0004-6361/202141152⟩
Astronomy and Astrophysics-A&A, 2021, 656, pp.A122. ⟨10.1051/0004-6361/202141152⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 656, pp.A122. ⟨10.1051/0004-6361/202141152⟩
We examine the dynamics of low-frequency gravito-inertial waves (GIWs) in differentially rotating deformed radiation zones in stars and planets by generalising the traditional approximation of rotation (TAR). The TAR treatment was built on the assump
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e9088eb601dc32fb277627d806b24ede
https://hal-cea.archives-ouvertes.fr/cea-03475470/document
https://hal-cea.archives-ouvertes.fr/cea-03475470/document