Publications

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1701 Publications visible to you, out of a total of 1701

Abstract

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Authors: Ondřej Podsztavek, Alexander I. Jordan, Pavel Tvrdík, Kai L. Polsterer

Date Published: 2024

Publication Type: Journal

Abstract (Expand)

In systems biology and systems medicine data of many different types and obtained from manifold methods are used to set up computational models for simulations and predictions. These data need to be interoperable to integrate them into the models or use them for model validation. To achieve this, standards are crucial for structuring, describing, and associating models and data, as well as their respective parts, graphical visualization, and information about applied experimental or computational methods. Such standards also assist with describing how constituent parts interact together, or are linked, and how they are embedded in their environmental and experimental context.

Authors: Martin Golebiewski, Gerhard Mayer

Date Published: 2024

Publication Type: InCollection

Abstract

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Authors: Rami Alsulami, Sabrina Einecke, Gavin Rowell, Padric McGee, Miroslav D. Filipović, Ivo Rolf Seitenzahl, Milorad Stupar, Tiffany Anne Collins, Yasuo Fukui, Hidetoshi Sano

Date Published: 2024

Publication Type: Journal

Abstract

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Authors: Evans Kojo Owusu, Sven Buder, Ashley J. Ruiter, Ivo Rolf Seitenzahl, Nicolas Rodriguez-Segovia

Date Published: 2024

Publication Type: Journal

Abstract (Expand)

Photometric time series gathered by space telescopes such as CoRoT and Kepler allow to detect solar-like oscillations in red giant stars and to measure their global seismic constraints, which can be used to infer global stellar properties (e.g. masses, radii, and evolutionary states). Combining such precise constraints with photospheric abundances provides a means of testing mixing processes that occur inside red-giant stars. In this work, we conduct a detailed spectroscopic and seismic analysis of nine nearby (d < 200 pc) red giant stars observed by Kepler. Both seismic constraints and grid-based modelling approaches are used to determine precise fundamental parameters for those evolved stars. We compare distances and radii derived from Gaia Data Release 3 parallaxes with those inferred by a combination of seismic, spectroscopic, and photometric constraints. We find no deviations within errors bars, however the small sample size and the associated uncertainties are a limiting factor for such comparison. We use the period spacing of mixed modes to distinguish between ascending red-giants and red clump stars. Based on the evolutionary status, we apply corrections to the values of Δν for some stars, resulting in a slight improvement to the agreement between seismic and photometric distances. Finally, we couple constraints on detailed chemical abundances with the inferred masses, radii, and evolutionary states. Our results corroborate previous studies that show that observed abundances of lithium and carbon isotopic ratio are in contrast with predictions from standard models, giving robust evidence for the occurrence of additional mixing during the red-giant phase.

Authors: H R Coelho, A Miglio, T Morel, N Lagarde, D Bossini, W J Chaplin, S Degl’Innocenti, M Dell’Omodarme, R A Garcia, R Handberg, S Hekker, D Huber, M N Lund, S Mathur, P G Prada Moroni, B Mosser, A Serenelli, M Rainer, J D do Nascimento, E Poretti, P Mathias, G Valle, P Dal Tio, T Duarte

Date Published: 2024

Publication Type: Journal

Abstract

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Authors: Chen Zhou, Marlen Neubert, Yuri Koide, Yumeng Zhang, Van-Quan Vuong, Tobias Schlöder, Stefanie Dehnen, Pascal Friederich

Date Published: 2024

Publication Type: Journal

Abstract

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Authors: Haixia Chai, Michael Strube

Date Published: 6th Dec 2023

Publication Type: InProceedings

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