Author
Listed:
- Anne Dutrey
(Université de Bordeaux, LAB, UMR 5804, F-33270 Floirac, France
Centre National de la Recherche Scientifique (CNRS), LAB, UMR 5804, F-33270 Floirac, France)
- Emmanuel Di Folco
(Université de Bordeaux, LAB, UMR 5804, F-33270 Floirac, France
Centre National de la Recherche Scientifique (CNRS), LAB, UMR 5804, F-33270 Floirac, France)
- Stéphane Guilloteau
(Université de Bordeaux, LAB, UMR 5804, F-33270 Floirac, France
Centre National de la Recherche Scientifique (CNRS), LAB, UMR 5804, F-33270 Floirac, France)
- Yann Boehler
(Centro de Radioastronomia y Astrofisica (CRyA), University of Mexico, Apartado Postal 3-72, 58089 Morelia, Michoacan, Mexico)
- Jeff Bary
(Colgate University, 13 Oak Drive, Hamilton, New York 13346, USA)
- Tracy Beck
(Space Telescope Science Institute, 3700 San Martin Drive)
- Hervé Beust
(Institut de Planetologie et d’Astrophysique de Grenoble (IPAG), UMR 5274, BP 53, F-38041 Grenoble Cedex 9, France)
- Edwige Chapillon
(Université de Bordeaux, LAB, UMR 5804, F-33270 Floirac, France
Institut de RadioAstronomie Millimetrique (IRAM), 300 rue de la Piscine, F-38046 Saint Martin d’Hères, France)
- Fredéric Gueth
(Institut de RadioAstronomie Millimetrique (IRAM), 300 rue de la Piscine, F-38046 Saint Martin d’Hères, France)
- Jean-Marc Huré
(Université de Bordeaux, LAB, UMR 5804, F-33270 Floirac, France
Centre National de la Recherche Scientifique (CNRS), LAB, UMR 5804, F-33270 Floirac, France)
- Arnaud Pierens
(Université de Bordeaux, LAB, UMR 5804, F-33270 Floirac, France
Centre National de la Recherche Scientifique (CNRS), LAB, UMR 5804, F-33270 Floirac, France)
- Vincent Piétu
(Institut de RadioAstronomie Millimetrique (IRAM), 300 rue de la Piscine, F-38046 Saint Martin d’Hères, France)
- Michal Simon
(Stony Brook University)
- Ya-Wen Tang
(Academia Sinica Institute of Astronomy and Astrophysics, PO Box 23-141, Taipei 106, Taiwan)
Abstract
Investigation of the triple stellar system GG Tau A reveals gas fragments within the central cavity between the Keplerian outer ring orbiting the entire system and the stars themselves; gas flow from this outer ring appears capable of sustaining the inner disk surrounding component star GG Tau Aa beyond the accretion lifetime, leaving time for planet formation to occur.
Suggested Citation
Anne Dutrey & Emmanuel Di Folco & Stéphane Guilloteau & Yann Boehler & Jeff Bary & Tracy Beck & Hervé Beust & Edwige Chapillon & Fredéric Gueth & Jean-Marc Huré & Arnaud Pierens & Vincent Piétu & Mich, 2014.
"Possible planet formation in the young, low-mass, multiple stellar system GG Tau A,"
Nature, Nature, vol. 514(7524), pages 600-602, October.
Handle:
RePEc:nat:nature:v:514:y:2014:i:7524:d:10.1038_nature13822
DOI: 10.1038/nature13822
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