Zobrazeno 1 - 10
of 334
pro vyhledávání: '"rotation [Stars]"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Blue supergiants (BSGs) are important objects to study the intermediate phases of massive star evolution, helping to constrain evolutionary models. However, the lack of a holistic study of a statistically significant and unbiased sample of these obje
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1078b1dcb9ecfbbd86cb84e6cc341933
http://arxiv.org/abs/2305.00305
http://arxiv.org/abs/2305.00305
Auxiliary data associated with the article "Constraints on Tidal Quality Factor in Kepler Eclipsing Binaries using Tidal Synchronization: A Frequency-Dependent Approach" by Patel, R., Penev, K. and Schussler J. The contents of the files are as follow
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1809008b11c0ecf27b5f6a280e095d25
Autor:
S. R. Berlanas, J. Maíz Apellániz, A. Herrero, L. Mahy, R. Blomme, I. Negueruela, R. Dorda, F. Comerón, E. Gosset, M. Pantaleoni González, J. A. Molina Lera, A. Sota, T. Furst, E. J. Alfaro, M. Bergemann, G. Carraro, J. E. Drew, L. Morbidelli, J. S. Vink
Publikováno v:
Berlanas, S R, Apellaniz, J M, Herrero, A, Mahy, L, Blomme, R, Negueruela, I, Dorda, R, Comeron, F, Gosset, E, Gonzalez, M P, Lera, J A M, Sota, A, Furst, T, Alfaro, E J, Bergemann, M, Carraro, G, Drew, J E, Morbidelli, L & Vink, J S 2023, ' Gaia-ESO survey : Massive stars in the Carina Nebula I. A new census of OB stars ', Astronomy & Astrophysics, vol. 671, A20 . https://doi.org/10.1051/0004-6361/202245335
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0727e8aa36812147951783acc8f3279c
http://hdl.handle.net/10261/310372
http://hdl.handle.net/10261/310372
Autor:
David Pamos Ortega, Antonio García Hernández, Juan Carlos Suárez, Javier Pascual Granado, Sebastià Barceló Forteza, José Ramón Rodón
Publikováno v:
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
ACKNOWLEDGEMENTS This publication is part of the project ‘Contribution of the UGR to the PLATO2.0 space mission. Phases C / D-1’, funded by MCNI/AEI/PID2019-107061GB-C64. DPO acknowledges MNRAS for the opportunity to publish his first scientific
Context. Gravito-inertial asteroseismology came into existence thanks to high-precision CoRoT and Kepler space photometric light curves. So far, it has given rise to the internal rotation frequency of a few hundred intermediate-mass stars, yet only s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______105::abd27f9ad807478304cdb0e64e658ab7
http://hdl.handle.net/1942/40570
http://hdl.handle.net/1942/40570
Classical T Tauri stars (CTTs) are young (a few Myr old) magnetized stellar objects that are accreting from their surroundings disks. Previous numerical studies have demonstrated that accretion in CTTs occurs in two different states: stable or unstab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1068748e8292f6b6477963e62697dab7
Publikováno v:
RID-UNRN (UNRN)
Universidad Nacional de Río Negro
instacron:UNRN
Universidad Nacional de Río Negro
instacron:UNRN
Fil: Ghoreyshi, Maziar. University of Western Ontario. Department of Physics and Astronomy. Ontario, Canada. Fil: Jones, Carol E. University of Western Ontario. Department of Physics and Astronomy. Ontario, Canada. Fil: Granada, Anahi. Universidad Na
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b27e24b5cfb2cd4e9a81bca7f0ca6a27
http://arxiv.org/abs/2210.14885
http://arxiv.org/abs/2210.14885
Autor:
Z Keszthelyi, A de Koter, Y Götberg, G Meynet, S A Brands, V Petit, M Carrington, A David-Uraz, S T Geen, C Georgy, R Hirschi, J Puls, K J Ramalatswa, M E Shultz, A ud-Doula
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 517(2), 2028-2055. Oxford University Press
Magnetic fields can drastically change predictions of evolutionary models of massive stars via mass-loss quenching, magnetic braking, and efficient angular momentum transport, which we aim to quantify in this work. We use the MESA software instrument
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::41ed4858dd8b05fdbe9150cbe77feb7d
https://lirias.kuleuven.be/handle/20.500.12942/706503
https://lirias.kuleuven.be/handle/20.500.12942/706503
Autor:
Mirouh, Giovanni Marcello
Publikováno v:
Frontiers in Astronomy and Space Sciences. 9
Asteroseismology has opened a window on the internal physics of thousands of stars, by relating oscillation spectra properties to the internal physics of stars. Mode identification, namely the process of associating a measured oscillation frequency t