Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Siemen Burssens"'
Autor:
Daniel V. Cotton, Derek L. Buzasi, Conny Aerts, Jeremy Bailey, Siemen Burssens, May G. Pedersen, Dennis Stello, Lucyna Kedziora-Chudczer, Ain De Horta, Peter De Cat, Fiona Lewis, Sai Prathyusha Malla, Duncan J. Wright, Kimberly Bott
Publikováno v:
Nature Astronomy, 6, pp. 154-164
Nature Astronomy, 6, 154-164
Nature Astronomy, 6, 154-164
Here we report the detection of polarization variations due to nonradial modes in the beta Cephei star beta Crucis. In so doing we confirm 40-year-old predictions of pulsation-induced polarization variability and its utility in asteroseismology for m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7bbab4d3c6a7eef061766aaafbc50a66
https://doi.org/10.1038/s41550-021-01531-9
https://doi.org/10.1038/s41550-021-01531-9
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
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
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
https://lirias.kuleuven.be/handle/123456789/639116