Asteroseismology; Stars: evolution; Stars: interiors; Stars: rotation; Internal rotations; Markov chain Monte Carlo; Markov Chain Monte-Carlo; Momentum transports; Star: evolution; Stars: Interiors; Stars: Rotation; Stellar interior; Subgiants; Astronomy and Astrophysics; Space and Planetary Science
Abstract :
[en] Context. The measurement of the internal rotation of post-main-sequence stars using data from space-based photometry missions has demonstrated the need for an efficient angular momentum transport in stellar interiors. No clear solution has emerged so far, and it remains a challenge for stellar modellers to explain the observed trends. Aims. We constrained the shape of the internal rotation profile of six Kepler subgiants that were studied in details in 2014 and also the properties of the missing angular momentum transport process that acts in stellar interiors from Markov chain Monte Carlo (MCMC) inversions of the internal rotation. Methods. We applied a new MCMC inversion technique to existing Kepler subgiant targets and tested various shapes of the internal rotation profile of the six subgiants that were observed in 2014. We also constrained the limitations on the number of free parameters that can be used in the MCMC inversion, showing the limitations in the amount of information in the seismic data. Results. First, we show that large-scale fossil magnetic fields are not able to explain the internal rotation of subgiants, similarly to what was determined from detailed studies of Kepler red giants. We are also able to constrain the location of the transition in the internal rotation profile for the most evolved stars in the available set of subgiants. We find that some of them exhibit a transition that is located close to the border of the helium core, but one object exhibit a transition located much higher in radius. Conclusions. We conclude that various processes might be at play that would explain our observations, but a consistent detailed modelling of all available subgiants is required to reveal the physical nature of the angular momentum process, in particular, for the least evolved objects. In addition, it is paramount to increase the number of stars for which these inferences are possible (e.g. with the future PLATO mission) because they play a key role in validating candidates for the transport process.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Buldgen, Gaël ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie ; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Fellay, Loïc ; Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
Bétrisey, J. ; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Deheuvels, S.; IRAP, Université de Toulouse, CNRS, CNES, UPS, Toulouse, France
Farnir, Martin ; Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
Farrell, E.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Language :
English
Title :
Markov chain Monte Carlo inversions of the internal rotation of Kepler subgiants
ERC - European Research Council SNF - Schweizerischer Nationalfonds zur Förderung der wissenschaftlichen Forschung F.R.S.-FNRS - Fonds de la Recherche Scientifique
Funding text :
We thank the anonymous referee for their careful reading of the manuscript. G.B. and J.B. are funded by the SNF AMBIZIONE grant No 185805 (Seismic inversions and modelling of transport processes in stars). G.B. acknowledges funding from the Fonds de la Recherche Scientifique - FNRS. L.F. is supported by the Fonds de la Recherche Scientifique (FNRS) as a Research fellow. S.D. acknowledges support from from the project BEAMING ANR-18-CE31-0001 of the French National Research Agency (ANR) and from the Centre National d'Etudes Spatiales (CNES). M.F. is a Postdoctoral Researcher of the Fonds de la Recherche Scientifique - FNRS. E.F. is support by SNF grant number 200020_212124.We thank the anonymous referee for their careful reading of the manuscript. G.B. and J.B. are funded by the SNF AMBIZIONE grant No 185805 (Seismic inversions and modelling of transport processes in stars). G.B. acknowledges funding from the Fonds de la Recherche Scientifique \u2013 FNRS. L.F. is supported by the Fonds de la Recherche Scientifique (FNRS) as a Research fellow. S.D. acknowledges support from from the project BEAMING ANR-18-CE31-0001 of the French National Research Agency (ANR) and from the Centre National d\u2019Etudes Spatiales (CNES). M.F. is a Postdoctoral Researcher of the Fonds de la Recherche Scientifique \u2013 FNRS. E.F. is support by SNF grant number 200020_212124.
Foreman-Mackey, D., Hogg, D. W., Lang, D., & Goodman, J. 2013, PASP, 125, 306
Fuller, J., Piro, A. L., & Jermyn, A. S. 2019, MNRAS, 485, 3661
García, R. A., Ceillier, T., Salabert, D., et al. 2014, A&A, 572, A34
Gehan, C., Mosser, B., Michel, E., Samadi, R., & Kallinger, T. 2018, A&A, 616, A24
Gelman, A., Carlin, J., Stern, H., et al. 2013, Bayesian Data Analysis, Third Edition, Chapman & Hall/CRC Texts in Statistical Science (Taylor & Francis)
Gough, D. O. 1981, MNRAS, 196, 731
Gough, D. O., & McIntyre, M. E. 1998, Nature, 394, 755
Goupil, M. J., Catala, C., Samadi, R., et al. 2024, A&A, 683, A78
Hansen, C. J., Cox, J. P., & van Horn, H. M. 1977, ApJ, 217, 151
Hatta, Y., Sekii, T., Takata, M., & Kurtz, D. W. 2019, ApJ, 871, 135