Weighing stars from birth to death: mass determination methods across the HRD

Autor: Paul G. Beck, M. G. Pedersen, Maria Bergemann, Vincent Van Eylen, Ignasi Ribas, Conny Aerts, Ian Czekala, Nicolas Lodieu, Eline Tolstoy, Marie Martig, Nate Bastian, Benard Nsamba, Davide Gandolfi, Ana Escorza, Keivan G. Stassun, Aldo Serenelli, George C. Angelou, Y. Lebreton, J. M. Bestenlehner, A. Moya, Krešimir Pavlovski, Achim Weiss, M. M. Miller Bertolami, J. S. G. Mombarg, D. Baroch, Victor Silva Aguirre, Diane Feuillet, Fabian Schneider, Juan Carlos Morales, Konstanze Zwintz, Mark Gieles, Nancy Elias-Rosa, Léo Girardi, Pier-Emmanuel Tremblay

Publikováno v: The Astronomy and Astrophysics Review, 29, 1-141
The Astronomy and Astrophysics Review
Astronomy and Astrophysics Review
Astronomy and Astrophysics Review, Springer Verlag, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Serenelli, A, Weiss, A, Aerts, C, Angelou, G C, Baroch, D, Bastian, N, Beck, P G, Bergemann, M, Bestenlehner, J M, Czekala, I, Elias-Rosa, N, Escorza, A, Van Eylen, V, Feuillet, D K, Gandolfi, D, Gieles, M, Girardi, L, Lebreton, Y, Lodieu, N, Martig, M, Miller Bertolami, M M, Mombarg, J S G, Morales, J C, Moya, A, Nsamba, B, Pavlovski, K, Pedersen, M G, Ribas, I, Schneider, F R N, Silva Aguirre, V, Stassun, K G, Tolstoy, E, Tremblay, P E & Zwintz, K 2021, ' Weighing stars from birth to death : mass determination methods across the HRD ', Astronomy and Astrophysics Review, vol. 29, no. 1, 4 . https://doi.org/10.1007/s00159-021-00132-9
Astronomy and Astrophysics Review, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
The Astronomy and Astrophysics Review, 29, 1, pp. 1-141

The mass of a star is the most fundamental parameter for its structure, evolution, and final fate. It is particularly important for any kind of stellar archaeology and characterization of exoplanets. There exist a variety of methods in astronomy to e

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0989a27c3e883ec587ab4cf7d39bff9c
http://sedici.unlp.edu.ar/handle/10915/132501

Forward seismic modeling of the pulsating magnetic B-type star HD43317

Autor: Cole Johnston, Dominic M. Bowman, B. Buysschaert, T. Van Reeth, Conny Aerts, C. Neiner, Stéphane Mathis, M. G. Pedersen

Publikováno v: Astronomy & Astrophysics
Astronomy & Astrophysics, 616, 1-19
Astronomy & Astrophysics, 616, pp. 1-19
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 616, pp.A148. ⟨10.1051/0004-6361/201832642⟩

The large-scale magnetic fields detected at the surface of about 10% of hot stars extend into the stellar interior, where they may alter the structure. Deep inner regions of stars are only observable using asteroseismology. Here, we investigated the

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f881660d9258611b12efd80c0b3a0a10
https://hdl.handle.net/2066/195374

The mass discrepancy in intermediate- and high-mass eclipsing binaries: The need for higher convective core masses

Autor: K. Pavlovski, V. Tsymbal, John Southworth, Mathias Michielsen, M. G. Pedersen, Dominic M. Bowman, Andrew Tkachenko, Cole Johnston, Conny Aerts

Publikováno v: Astronomy and Astrophysics
Volume 637
Astronomy & Astrophysics, 637, pp. 1-20
Astronomy & Astrophysics, 637, 1-20
Astronomy & Astrophysics

(Abridged) Eclipsing, spectroscopic double-lined binary star systems (SB2) are excellent laboratories for calibrating theories of stellar interior structure and evolution. We aim to investigate the mass discrepancy in binary stars. We study the effec

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63b6489719c0c76d7c4dcc6b963dec6e
https://doi.org/10.1051/0004-6361/202037452

Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry

Autor: Norberto Castro, Dominic M. Bowman, R. P. Ratnasingam, Ehsan Moravveji, Sergio Simón-Díaz, Mathias Michielsen, Siemen Burssens, Benjamin J. S. Pope, Peter De Cat, Conny Aerts, B. Buysschaert, Timothy R. White, Tamara M. Rogers, M. G. Pedersen, Cole Johnston, Andrew Tkachenko, P. V. F. Edelmann

Publikováno v: Nature Astronomy, 3, 760-765
Nature Astronomy
Nature Astronomy, 3, 8, pp. 760-765

Almost all massive stars explode as supernovae and form a black hole or neutron star. The remnant mass and the impact of the chemical yield on subsequent star formation and galactic evolution strongly depend on the internal physics of the progenitor

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7367667d64be06cf0d074d1979beaec
https://lirias.kuleuven.be/handle/123456789/639116

Diverse Variability of O and B Stars Revealed from 2-minute Cadence Light Curves in Sectors 1 and 2 of the TESS Mission: Selection of an Asteroseismic Sample

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

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/