Protoplanetary Disks as seen by Interferometry
DUTREY, Anne
Laboratoire d'Astrophysique de Grenoble [LAOG]
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Laboratoire d'Astrophysique de Grenoble [LAOG]
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
DUTREY, Anne
Laboratoire d'Astrophysique de Grenoble [LAOG]
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
< Leer menos
Laboratoire d'Astrophysique de Grenoble [LAOG]
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Idioma
en
Communication dans un congrès
Este ítem está publicado en
The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation, Eso Astrophysics Symposia, Volume . ISBN 978-3-540-74253-1. Springer, 2008, The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation, Eso Astrophysics Symposia, Volume . ISBN 978-3-540-74253-1. Springer, 2008, Proceedings of the ESO Workshop held in Garching, Germany, 4-8 April 2005, 2005. 2008p. 217
Resumen en inglés
Protoplanetary disks encountered around young Pre-Main-Sequence(PMS) stars of low or intermediate masses are now observable bycurrent Near-Infrared (NIR) and Mid-Infrared interferometers.Taking also into account the progress ...Leer más >
Protoplanetary disks encountered around young Pre-Main-Sequence(PMS) stars of low or intermediate masses are now observable bycurrent Near-Infrared (NIR) and Mid-Infrared interferometers.Taking also into account the progress done by millimeter arrays, interferometry is slowly but surely changing the knowledge we have of their physics. In this review, I show how these recent observations help to constrain the physical properties of both the very inner disks where planetary formation should occur and the outer disk where the reservoir of mass is located. I also illustrate this by presenting interferometric studies from a fewexamples such as AB Auriga< Leer menos
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