Sign on
ADS Classic is now deprecated. It will be completely retired in October 2019. This page will automatically redirect to the new ADS interface at that point.

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Full Printable Article (PDF/Postscript)
· Scanned Article (GIF)
· Table of Contents
· References in the Article
· Citations to the Article (2) (Citation History)
· Refereed Citations to the Article
· Reads History
·
· Translate This Page
Title:
The planet companion around beta Pictoris
Authors:
Lagrange, Anne-Marie; Bonnefoy, Mickaël; Chauvin, Gael; Apai, Daniel; Ehrenreich, David; Boccaletti, Anthony; Gratadour, Damien; Rouan, Daniel; Mouillet, David; Lacour, Sylvestre; Kasper, Markus
Affiliation:
AA(Laboratoire dAstrophysique de Grenoble, France ), AB(Laboratoire dAstrophysique de Grenoble, France ), AC(Laboratoire dAstrophysique de Grenoble, France ), AD(Space Telesope Sciente Institute, 3700 San Martin Dr. Baltimore, MD 21218, USA ), AE(Laboratoire dAstrophysique de Grenoble, France ), AF(LESIA, Observatoire de Paris, place Jules Janssen, 92195 Meudon, France ), AG(LESIA Observatoire de Paris, place Jules Janssen, 92195 Meudon, France ), AH(LESIA Observatoire de Paris, place Jules Janssen, 92195 Meudon, France ), AI(Laboratoire dAstrophysique de Grenoble, France ), AJ(LESIA, Observatoire de Paris, place Jules Janssen, 92195 Meudon, France ), AK(ESO, Karl Schwarzschild St, 2, 85748 Garching bei Muenchen, Germany )
Publication:
The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution, Proceedings of the International Astronomical Union, IAU Symposium, Volume 276, p. 60-63
Publication Date:
11/2011
Origin:
CUP
Keywords:
planetary systems: formation, techniques: high angular resolution
Abstract Copyright:
(c) 2011: Copyright © International Astronomical Union 2011
DOI:
10.1017/S1743921311019946
Bibliographic Code:
2011IAUS..276...60L

Abstract

The beta Pic disk of dust and gas has been regarded as the prototype of young planetary systems since the 1980s and has revealed over the years an impressive amount of indirect signs pointing toward the presence of at least one giant planet. We present here the recently detected first giant planet around this star. We show how this planet could explain some very peculiar features of the star environment (disk, spectroscopic variability), and how it constrains the scenarios of planetary system formation (timescales, mechanisms).

Printing Options

Print whole paper
Print Page(s) through

Return 600 dpi PDF to Acrobat/Browser. Different resolutions (200 or 600 dpi), formats (Postscript, PDF, etc), page sizes (US Letter, European A4, etc), and compression (gzip,compress,none) can be set through the Printing Preferences



More Article Retrieval Options

HELP for Article Retrieval


Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)


Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints