Zobrazeno 1 - 10
of 2 725
pro vyhledávání: '"Müllner, M"'
Publikováno v:
A&A 664, A32 (2022)
The physics of early stellar evolution (e.g. accretion processes) is often not properly included in the calculations of pre-main-sequence models, leading to insufficient model grids and hence systematic errors in the results. We aim to investigate cu
Externí odkaz:
http://arxiv.org/abs/2206.07317
Publikováno v:
A&A 654, A36 (2021)
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
Externí odkaz:
http://arxiv.org/abs/2107.07568
Autor:
Müllner, M., Zwintz, K., Corsaro, E., Steindl, T., Potravnov, I., Guenther, E. W., Kniazev, A., Gvaramadze, V.
Publikováno v:
A&A 647, A168 (2021)
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 around the observationa
Externí odkaz:
http://arxiv.org/abs/2012.07878
Autor:
Zwintz, K., Neiner, C., Kochukhov, O., Rybchikova, T., Pigulski, A., Muellner, M., Steindl, T., Kuschnig, R., Handler, G., Moffat, A. F. J., Pablo, H., Popowicz, A., Wade, G. A.
Publikováno v:
A&A 643, A110 (2020)
F type stars are characterised by several physical processes such as different pulsation mechanisms, rotation, convection, diffusion, and magnetic fields. The rapidly rotating delta Scuti star beta Cas can be considered as a benchmark star to study t
Externí odkaz:
http://arxiv.org/abs/2009.04784
Autor:
Zwintz, K., Reese, D. R., Neiner, C., Pigulski, A., Kuschnig, R., Muellner, M., Zieba, S., Abe, L., Guillot, T., Handler, G., Kenworthy, M., Stuik, R., Moffat, A. F. J., Popowicz, A., Rucinski, S. M., Wade, G. A., Weiss, W. W., Bailey III, J. I., Crawford, S., Ireland, M., Kuhn, R., Lomberg, B., Mamajek, E. E., Mellon, S. N., Talens, G. J.
Publikováno v:
A&A 627, A28 (2019)
Exoplanet properties crucially depend on their host stars' parameters. In case the exoplanet host star shows pulsations, asteroseismology can be used for an improved description of the stellar parameters. We aim to revisit the pulsational properties
Externí odkaz:
http://arxiv.org/abs/1905.12545
Autor:
Leslie KG; Department of Chemistry, Durham University, Durham DH1 3LE, U.K.; School of Chemistry University of Sydney, Sydney, NSW 2006, Australia., Jolliffe KA; School of Chemistry University of Sydney, Sydney, NSW 2006, Australia.; Australian Research Council Centre of Excellence for Innovations in Peptide and Protein Science, University of Sydney, Sydney, NSW 2006, Australia.; Sydney Nano Institute, University of Sydney, Sydney, NSW 2006, Australia., Müllner M; School of Chemistry University of Sydney, Sydney, NSW 2006, Australia.; Key Centre for Polymers and Colloids, School of Chemistry, University of Sydney, Sydney, NSW 2006, Australia.; Sydney Nano Institute, University of Sydney, Sydney, NSW 2006, Australia., New EJ; School of Chemistry University of Sydney, Sydney, NSW 2006, Australia.; Australian Research Council Centre of Excellence for Innovations in Peptide and Protein Science, University of Sydney, Sydney, NSW 2006, Australia.; Sydney Nano Institute, University of Sydney, Sydney, NSW 2006, Australia., Turnbull WB; School of Chemistry and Astbury Centre for Structural Molecular Biology, University of Leeds, Leeds LS2 9JT, U.K., Fascione MA; Department of Chemistry and York Structural Biology Laboratory, University of York, York YO10 5DD, U.K., Friman VP; Department of Biology, University of York, York YO10 5DD, U.K.; Department of Microbiology, Faculty of Agriculture and Forestry, University of Helsinki, Helsinki FI-00014, Finland.; Viikki Biocenter, University of Helsinki, POB 56, Helsinki FI-00014, Finland., Mahon CS; Department of Chemistry, Durham University, Durham DH1 3LE, U.K.; School of Chemistry University of Sydney, Sydney, NSW 2006, Australia.
Publikováno v:
Biomacromolecules [Biomacromolecules] 2024 Nov 11; Vol. 25 (11), pp. 7466-7474. Date of Electronic Publication: 2024 Oct 18.
Autor:
Gogoi N; ARC Training Centre for Future Crops Development, Research School of Biology, College of Science, The Australian National University, Canberra, ACT 2601, Australia. Electronic address: neelam.gogoi@anu.edu.au., Susila H; ARC Training Centre for Future Crops Development, Research School of Biology, College of Science, The Australian National University, Canberra, ACT 2601, Australia., Leach J; ARC Training Centre for Future Crops Development, Research School of Biology, College of Science, The Australian National University, Canberra, ACT 2601, Australia; Australian National Centre for the Public Awareness of Science, The Australian National University, Canberra, ACT 2601, Australia., Müllner M; Key Centre for Polymers & Colloids, School of Chemistry, Faculty of Science, The University of Sydney, NSW 2006, Australia; Sydney Institute of Agriculture, The University of Sydney, NSW 2006, Australia; The University of Sydney Nano Institute (Sydney Nano), The University of Sydney, NSW 2006, Australia., Jones B; Sydney Institute of Agriculture, The University of Sydney, NSW 2006, Australia; School of Life and Environmental Sciences, Faculty of Science, The University of Sydney, Camperdown, NSW 2006, Australia., Pogson BJ; ARC Training Centre for Future Crops Development, Research School of Biology, College of Science, The Australian National University, Canberra, ACT 2601, Australia. Electronic address: barry.pogson@anu.edu.au.
Publikováno v:
Trends in plant science [Trends Plant Sci] 2024 Oct 29. Date of Electronic Publication: 2024 Oct 29.
Autor:
Müllner, M., Schröder, W.
Publikováno v:
In Journal of Computational Physics 15 July 2020 413
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