Asteroseismology. Echography of young stars reveals their evolution

Autor: K, Zwintz, L, Fossati, T, Ryabchikova, D, Guenther, C, Aerts, T G, Barnes, N, Themeßl, D, Lorenz, C, Cameron, R, Kuschnig, S, Pollack-Drs, E, Moravveji, A, Baglin, J M, Matthews, A F J, Moffat, E, Poretti, M, Rainer, S M, Rucinski, D, Sasselov, W W, Weiss

Publikováno v: Science (New York, N.Y.). 345(6196)

We demonstrate that a seismic analysis of stars in their earliest evolutionary phases is a powerful method with which to identify young stars and distinguish their evolutionary states. The early star that is born from the gravitational collapse of a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=pmid________::dd905ddc89bf2d668dde8ff25cee549c
https://pubmed.ncbi.nlm.nih.gov/25082686

Asteroseismology. Echography of young stars reveals their evolution.

Autor: Zwintz K; Instituut voor Sterrenkunde, Katholieke Universiteit (KU) Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium. konstanze.zwintz@ster.kuleuven.be., Fossati L; Argelander Institut für Astronomie der Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany., Ryabchikova T; Institute of Astronomy, Russian Academy of Sciences (RAS), Pyatnitskaya 48, 109017 Moscow, Russia., Guenther D; Department of Astronomy and Physics, St. Mary's University, Halifax, Nova Scotia B3H 3C3, Canada., Aerts C; Instituut voor Sterrenkunde, Katholieke Universiteit (KU) Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium. Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen, Post Office Box 9010, 6500 GL Nijmegen, Netherlands., Barnes TG; The University of Texas at Austin, McDonald Observatory, 82 Mt. Locke Road, McDonald Observatory, TX 79734, USA., Themeßl N; Universität Wien, Institut für Astrophysik, Türkenschanzstraße 17, 1180 Vienna, Austria., Lorenz D; Universität Wien, Institut für Astrophysik, Türkenschanzstraße 17, 1180 Vienna, Austria., Cameron C; Department of Mathematics, Physics and Geology, Cape Breton University, 1250 Grand Lake Road, Sydney, Nova Scotia B1P 6L2, Canada., Kuschnig R; Universität Wien, Institut für Astrophysik, Türkenschanzstraße 17, 1180 Vienna, Austria., Pollack-Drs S; Universität Wien, Institut für Astrophysik, Türkenschanzstraße 17, 1180 Vienna, Austria., Moravveji E; Instituut voor Sterrenkunde, Katholieke Universiteit (KU) Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium., Baglin A; Laboratoire d'Études Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris-Meudon, 5 place Jules Janssen, 92195, Meudon, France., Matthews JM; Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia V6T 1Z1, Canada., Moffat AF; Départment de Physique, Université de Montréal, C.P. 6128, Succ. Centre-Ville, Montréal, Quebec H3C 3J7, Canada., Poretti E; Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807 Merate, Italy., Rainer M; Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807 Merate, Italy., Rucinski SM; Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, Ontario M5S 3H4, Canada., Sasselov D; Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA., Weiss WW; Universität Wien, Institut für Astrophysik, Türkenschanzstraße 17, 1180 Vienna, Austria.

Publikováno v: Science (New York, N.Y.) [Science] 2014 Aug 01; Vol. 345 (6196), pp. 550-3. Date of Electronic Publication: 2014 Jul 03.