Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Timothy, Van Reeth"'
Spinning up the Surface: Evidence for Planetary Engulfment or Unexpected Angular Momentum Transport?
Autor:
Jamie Tayar, Facundo D. Moyano, Melinda Soares-Furtado, Ana Escorza, Meridith Joyce, Sarah L. Martell, Rafael A. García, Sylvain N. Breton, Stéphane Mathis, Savita Mathur, Vincent Delsanti, Sven Kiefer, Sabine Reffert, Dominic M. Bowman, Timothy Van Reeth, Shreeya Shetye, Charlotte Gehan, Samuel K. Grunblatt
Publikováno v:
The Astrophysical Journal, Vol 940, Iss 1, p 23 (2022)
In this paper, we report the potential detection of a nonmonotonic radial rotation profile in a low-mass lower-luminosity giant star. For most low- and intermediate-mass stars, the rotation on the main sequence seems to be close to rigid. As these st
Externí odkaz:
https://doaj.org/article/6001f52a1aa9479f86e2d63223f3da31
Autor:
Timothy Van Reeth, John Southworth
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 515:2755-2765
The study of pulsating stars in eclipsing binaries holds the promise of combining two different ways of measuring the physical properties of a star to obtain improved constraints on stellar theory. Gravity (g) mode pulsations such as those found in $
Autor:
Gang Li, Joey S. G. Mombarg, Peter De Cat, Patricia Lampens, Andrew Tkachenko, M. G. Pedersen, Timothy Van Reeth, J. Bodensteiner, Ilya Straumit, Hans-Walter Rix, Conny Aerts, L. Vermeylen, Ana Escorza, Dominic M. Bowman, Sarah Gebruers
Publikováno v:
Gebruers, S, Straumit, I, Tkachenko, A, Mombarg, J S G, Pedersen, M G, Van Reeth, T, Li, G, Lampens, P, Escorza, A, Bowman, D M, De Cat, P, Vermeylen, L, Bodensteiner, J, Rix, H W & Aerts, C 2021, ' A homogeneous spectroscopic analysis of a Kepler legacy sample of dwarfs for gravity-mode asteroseismology ', Astronomy and Astrophysics, vol. 650, A151 . https://doi.org/10.1051/0004-6361/202140466
Astronomy & Astrophysics, 650, pp. 1-27
Astronomy & Astrophysics, 650, 1-27
Astronomy & Astrophysics
Astronomy & Astrophysics, 650, pp. 1-27
Astronomy & Astrophysics, 650, 1-27
Astronomy & Astrophysics
Asteroseismic modelling of the internal structure of main-sequence stars born with a convective core has so far been based on homogeneous analyses of space photometric Kepler light curves of 4 years duration, to which most often incomplete inhomogene
Context. Many well-known bright stars have been observed by the ongoing Transiting Exoplanet Survey Satellite (TESS) space mission. For several of them, these new data reveal previously unobserved variability, such as tidally perturbed pulsations in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fc46566b82fbcf177643e75a77c854ea
http://arxiv.org/abs/2201.05359
http://arxiv.org/abs/2201.05359
Autor:
Sarah Gebruers, Andrew Tkachenko, Dominic M. Bowman, Timothy Van Reeth, Siemen Burssens, Luc IJspeert, Laurent Mahy, Ilya Straumit, Maosheng Xiang, Hans-Walter Rix, Conny Aerts
Publikováno v:
Astronomy & Astrophysics, 665, 1-17
Astronomy & Astrophysics, 665, pp. 1-17
Astronomy & Astrophysics, 665, pp. 1-17
Spectroscopic data are necessary to break degeneracies in asteroseismic modelling of the interior structure in high- and intermediate-mass stars. We derive precise photospheric stellar parameters for a sample of 166 B-type stars with TESS light curve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::86d799c462fdfeaea018aeb9e469012e
Publikováno v:
Barbara, N H, Bedding, T R, Fulcher, B D, Murphy, S J & Van Reeth, T 2022, ' Classifying Kepler light curves for 12 000 A and F stars using supervised feature-based machine learning ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 2, pp. 2793-2804 . https://doi.org/10.1093/mnras/stac1515
With the availability of large-scale surveys like Kepler and TESS, there is a pressing need for automated methods to classify light curves according to known classes of variable stars. We introduce a new algorithm for classifying light curves that co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::053bc37bda8527fbf9adb4230a667b85
About 10 per cent of intermediate- and high-mass dwarf stars are observed to host a strong large-scale magnetic field at their surface, which is thought to be of fossil field origin. However, there are few inferences as to the magnetic field strength
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0e663ad8f15f07dcd52c6d81f855d93
Autor:
Timothy Van Reeth, Rasmus Handberg, Derek Buzasi, Mikkel N. Lund, Oliver J. Hall, Filipe Pereira, Daniel Huber, Lindsey Carboneau, Daniel R. Hey
Publikováno v:
Lund, M N, Handberg, R, Buzasi, D L, Carboneau, L, Hall, O J, Pereira, F, Huber, D, Hey, D, Van Reeth, T & The T'DA Collaboration 2021, ' TESS Data for Asteroseismology : Light-curve Systematics Correction ', Astrophysical Journal, Supplement Series, vol. 257, no. 2, 53 . https://doi.org/10.3847/1538-4365/ac214a
Data from the Transiting Exoplanet Survey Satellite (TESS) has produced of order one million light curves at cadences of 120 s and especially 1800 s for every ~27-day observing sector during its two-year nominal mission. These data constitute a treas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69947d99d9e4ed422d95e5b7983ebfb2
https://pure.au.dk/portal/da/publications/tess-data-for-asteroseismology(2dca7cc8-63db-4901-b985-e291531450e9).html
https://pure.au.dk/portal/da/publications/tess-data-for-asteroseismology(2dca7cc8-63db-4901-b985-e291531450e9).html
The relation of period spacing ($\Delta P$) versus period ($P$) of dipole prograde g modes is known to be useful to measure rotation rates in the g-mode cavity of rapidly rotating $\gamma$ Dor and slowly pulsating B (SPB) stars. In a rapidly rotating
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5bf24a0df1863346605bcc22a5b486e3
https://lirias.kuleuven.be/handle/123456789/675367
https://lirias.kuleuven.be/handle/123456789/675367
Autor:
Aaron Dotter, Timothy Van Reeth, Andrew Tkachenko, Sarah Gebruers, J. S. G. Mombarg, Conny Aerts
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 895, 1-17
The Astrophysical Journal, 895, 1, pp. 1-17
The Astrophysical Journal, 895, 1-17
The Astrophysical Journal, 895, 1, pp. 1-17
It has been known for several decades that transport of chemical elements is induced by the process of microscopic atomic diffusion. Yet, the effect of atomic diffusion, including radiative levitation, has hardly been studied in the context of gravit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ff97d09882a5af3182ae988805b2baf
https://lirias.kuleuven.be/handle/123456789/656299
https://lirias.kuleuven.be/handle/123456789/656299