Zobrazeno 1 - 10
of 13
pro vyhledávání: '"G. M. Mirouh"'
Autor:
Nina S Sartorio, A Fialkov, T Hartwig, G M Mirouh, R G Izzard, M Magg, R S Klessen, S C O Glover, L Chen, Y Tarumi, D D Hendriks
The first population of X-ray binaries (XRBs) is expected to affect the thermal and ionization states of the gas in the early Universe. Although these X-ray sources are predicted to have important implications for high-redshift observable signals, su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0cc384ccd691420171211cdf5130e1d
Autor:
T Gessey-Jones, N S Sartorio, A Fialkov, G M Mirouh, M Magg, R G Izzard, E de Lera Acedo, W J Handley, R Barkana
Properties of the first generation of stars [referred to as the Population III (Pop III) stars], such as their initial mass function (IMF), are poorly constrained by observations and have yet to converge between simulations. The cosmological 21-cm si
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28bfaf4f173aeb70a4ccad23d39939ab
http://arxiv.org/abs/2202.02099
http://arxiv.org/abs/2202.02099
Autor:
Dogus Ozuyar, Alexandre David-Uraz, Gregg A. Wade, S. Chowdhury, Matteo Cantiello, C. A. Engelbrecht, L. A. Balona, Gerald Handler, G. M. Mirouh
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 485:3457-3469
Light curves and periodograms of 160 B stars observed by the TESS space mission and 29 main-sequence B stars from Kepler and K2 were used to classify the variability type. There are 114 main-sequence B stars in the TESS sample, of which 45 are classi
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
Autor:
Roland Vanderspek, Peter De Cat, Alexandre David-Uraz, Jadwiga Daszyńska-Daszkiewicz, Dominic M. Bowman, Matteo Cantiello, Derek Buzasi, George R. Ricker, Coralie Neiner, Catherine Lovekin, Conny Aerts, Andrew Tkachenko, M. G. Pedersen, Andrzej Pigulski, James Sikora, S. Chowdhury, Gerald Handler, Sergio Simón-Díaz, G. M. Mirouh, Cole Johnston, Ehsan Moravveji
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2019, 872 (1), pp.L9. ⟨10.3847/2041-8213/ab01e1⟩
The Astrophysical Journal, 872, 1, pp. 1-16
The Astrophysical Journal, 872, 1-16
The Astrophysical Journal
The Astrophysical journal letters, Bristol : IOP Publishing, 2019, 872 (1), pp.L9. ⟨10.3847/2041-8213/ab01e1⟩
The Astrophysical Journal, 872, 1, pp. 1-16
The Astrophysical Journal, 872, 1-16
The Astrophysical Journal
Uncertainties in stellar structure and evolution theory are largest for stars undergoing core convection on the main sequence. A powerful way to calibrate the free parameters used in the theory of stellar interiors is asteroseismology, which provides
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1668431b6e95db91d84ed792ae7e916b
https://surrey.eprints-hosting.org/850710/
https://surrey.eprints-hosting.org/850710/
Asteroseismology of massive stars with the TESS mission: the runaway β Cep pulsator PHL 346 = HN Aqr
Autor:
Zhao Guo, Sergio Simón-Díaz, J. Pascual-Granado, Dominic M. Bowman, George R. Ricker, Filiz Kahraman Alicavus, Cole Johnston, M. G. Pedersen, Derek Buzasi, David Kilkenny, Thomas Kallinger, Peter De Cat, G. M. Mirouh, Tomasz Różański, Kosmas Gazeas, Ehsan Moravveji, S. Chowdhury, Jadwiga Daszyńska-Daszkiewicz, Gerald Handler, Norbert Przybilla, Ewa Niemczura, Andreas Irrgang, Roland Vanderspek, Andrzej Pigulski
Publikováno v:
The Astrophysical Journal
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
We report an analysis of the first known β Cep pulsator observed by the Transiting Exoplanet Survey Satellite (TESS) mission, the runaway star PHL 346 = HN Aqr. The star, previously known as a singly periodic pulsator, has at least 34 oscillation mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8c1bd97830e53c3e7fba6a2f3610079b
http://hdl.handle.net/10261/190649
http://hdl.handle.net/10261/190649
Publikováno v:
Journal of Fluid Mechanics
Journal of Fluid Mechanics, Cambridge University Press (CUP), 2016, 800, pp.213-247. ⟨10.1017/jfm.2016.382⟩
Journal of Fluid Mechanics, Cambridge University Press (CUP), 2016, 800, pp.213-247. ⟨10.1017/jfm.2016.382⟩
The gravito-inertial waves propagating over a shellular baroclinic flow inside a rotating spherical shell are analysed using the Boussinesq approximation. The wave properties are examined by computing paths of characteristics in the non-dissipative l
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2019, 483 (1), pp.L28-L32. ⟨10.1093/mnrasl/sly212⟩
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2019, 483 (1), pp.L28-L32. ⟨10.1093/mnrasl/sly212⟩
Oscillation modes in fast-rotating stars can be split into several subclasses, each with their own properties. To date, seismology of these stars cannot rely on regular pattern analysis and scaling relations. However, recently there has been the prom
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4991e85d4a0e556bf5b7d9bf1fbe5832
http://arxiv.org/abs/1811.05769
http://arxiv.org/abs/1811.05769
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 598, pp.A99. ⟨10.1051/0004-6361/201629274⟩
Astronomy and Astrophysics-A&A, 2017, 598, pp.A99. ⟨10.1051/0004-6361/201629274⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 598, pp.A99. ⟨10.1051/0004-6361/201629274⟩
Astronomy and Astrophysics-A&A, 2017, 598, pp.A99. ⟨10.1051/0004-6361/201629274⟩
As the global magnetic field of the Sun has an activity cycle, one expects to observe some variation of the dynamical properties of the flows visible in the photosphere. We investigate the flow field during the solar cycle by analysing SDO/HMI observ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63072b216109f99713ee49a1b4b6b192
https://hal.archives-ouvertes.fr/hal-02178065
https://hal.archives-ouvertes.fr/hal-02178065
Publikováno v:
EPJ Web of Conferences, Vol 101, p 06046 (2015)
Oscillations have been detected in a variety of stars, including intermediate- and high-mass main sequence stars. While many of these stars are rapidly and differentially rotating, the effects of rotation on oscillation modes are poorly known. In thi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8696d5c002e9ddad6fecd28e26ec16f7
https://surrey.eprints-hosting.org/852889/
https://surrey.eprints-hosting.org/852889/