Zobrazeno 1 - 10
of 47
pro vyhledávání: '"T. Steindl"'
Autor:
T Steindl-Schönhuber, G Gittler
Publikováno v:
Section 5: Patient safety and quality assurance.
The effects of an accretion disk are crucial to understanding the evolution of young stars. During the combined evolution, stellar and disk parameters influence each other, motivating a combined stellar and disk model. This makes a combined numerical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e477e21886b2eee19b365bd1c046e9f
http://arxiv.org/abs/2211.05331
http://arxiv.org/abs/2211.05331
Autor:
T Steindl-Schönhuber, G Gittler
Publikováno v:
Section 3: Production and compounding.
Akademický článek
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Publikováno v:
Astronomy & Astrophysics
Stellar components in binaries are subject to tidal forces which influence asteroseismic properties. Tidally pertubed pulsations have been reported for different objects but none of these are in their pre-main sequence phase of evolution. This makes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::73e4eb3a6a2ded3089452b5c031027a2
http://arxiv.org/abs/2011.08214
http://arxiv.org/abs/2011.08214
Autor:
Adam Popowicz, A. F. J. Moffat, M. Müllner, Oleg Kochukhov, Herbert Pablo, Rainer Kuschnig, K. Zwintz, Andrzej Pigulski, T. Steindl, Gregg A. Wade, T. A. Ryabchikova, Coralie Neiner, Gerald Handler
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A110. ⟨10.1051/0004-6361/202038210⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A110. ⟨10.1051/0004-6361/202038210⟩
Context. F-type stars are characterised by several physical processes such as different pulsation mechanisms, rotation, convection, diffusion, and magnetic fields. The rapidly rotating δ Scuti star β Cas can be considered as a benchmark star to stu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::049ae320b86da3e6ae73c0854520000c
https://hal.archives-ouvertes.fr/hal-03254112
https://hal.archives-ouvertes.fr/hal-03254112
Publikováno v:
Astronomy & Astrophysics. 654:A36
Context: The pre-main sequence evolution is often simplified by choosing classical initial models. These have large initial radii and sufficient uniform contraction to make them fully convective. Contrary to that, real stars are born as small protost
Autor:
Vasilii V. Gvaramadze, K. Zwintz, M. Müllner, E. W. Guenther, A. Y. Kniazev, Enrico Corsaro, T. Steindl, I. S. Potravnov
Publikováno v:
Astronomy & Astrophysics. 647:A168
Context. In recent years, our understanding of solar-like oscillations from main sequence to red giant stars has improved dramatically thanks to pristine data collected from space telescopes. One of the remaining open questions focuses on the observa
Akademický článek
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Publikováno v:
Aktuelle Ernährungsmedizin. 36:341-350
Fragestellung Die perkutane endoskopische Gastrostomie ist eine etablierte Methode fur die langerfristige enterale Ernahrung. Die Studie untersuchte Ernahrungszustand, Lebensqualitat und Situation von Patienten nach Sondenlegung sowie den Nutzen eine