Correlations between the stellar, planetary, and debris components of exoplanet systems observed by Herschel
Article
Article Title | Correlations between the stellar, planetary, and debris components of exoplanet systems observed by Herschel |
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ERA Journal ID | 1050 |
Article Category | Article |
Authors | Marshall, J. P. (Author), Moro-Martin, A. (Author), Eiroa, C. (Author), Kennedy, G. (Author), Mora, A. (Author), Sibthorpe, B. (Author), Lestrade, J. -F. (Author), Maldonado, J. (Author), Sanz-Forcada, J. (Author), Wyatt, M. C. (Author), Matthews, B. (Author), Horner, J. (Author), Montesinos, B. (Author), Bryden, G. (Author), Del Burgo, C. (Author), Greaves, J. S. (Author), Ivison, R. J. (Author), Meeus, G. (Author), Olofsson, G. (Author), Pilbratt, G. L. (Author) and White, G. J. (Author) |
Journal Title | Astronomy and Astrophysics: a European journal |
Journal Citation | 565, p. A15 |
Number of Pages | 14 |
Year | 2014 |
Publisher | EDP Sciences |
Place of Publication | Les Ulis, France |
ISSN | 0004-6361 |
1432-0746 | |
Digital Object Identifier (DOI) | https://doi.org/10.1051/0004-6361/201323058 |
Abstract | Context. Stars form surrounded by gas-and dust-rich protoplanetary discs. Generally, these discs dissipate over a few (3-10) Myr, leaving a faint tenuous debris disc composed of second-generation dust produced by the attrition of larger bodies formed in the protoplanetary disc. Giant planets detected in radial velocity and transit surveys of main-sequence stars also form within the protoplanetary disc, whilst super-Earths now detectable may form once the gas has dissipated. Our own solar system, with its eight planets and two debris belts, is a prime example of an end state of this process. |
Keywords | circumstellar matter; infrared; planetary systems; stars; planet-disk interactions |
ANZSRC Field of Research 2020 | 510109. Stellar astronomy and planetary systems |
519999. Other physical sciences not elsewhere classified | |
510101. Astrobiology | |
Public Notes | © 2014 ESO. This publication is copyright. It may be reproduced in whole or in part for the purposes of study, research, or review, but is subject to the inclusion of an acknowledgment of the source. |
Byline Affiliations | Autonomous University of Madrid, Spain |
Spanish Astrobiology Centre, Spain | |
University of Cambridge, United Kingdom | |
European Space Astronomy Centre, Spain | |
Netherlands Institute for Space Research, Netherlands | |
Paris Observatory, France | |
Herzberg Astronomy and Astrophysics Centre, Canada | |
Computational Engineering and Science Research Centre | |
California Institute of Technology (Caltech), United States | |
National Institute of Astrophysics Optics and Electronics, Mexico | |
University of St Andrews, United Kingdom | |
Royal Observatory Edinburgh, United Kingdom | |
Stockholm University, Sweden | |
European Space Agency, France | |
Open University, United Kingdom | |
Institution of Origin | University of Southern Queensland |
https://research.usq.edu.au/item/q2816/correlations-between-the-stellar-planetary-and-debris-components-of-exoplanet-systems-observed-by-herschel
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