The European Space Agency's Gaia space telescope, launched in 2013, aims to measure the positions, parallaxes, and proper motions of a billion stars in our Galaxy and throughout the Local Group. In doing so it will include hundreds of thousands of young stars in star forming regions, star clusters and OB associations. This will provide us with an unprecedented view of the role of dynamics in the star formation process and the evolution of young star clusters. Data from this ambitious mission is expected very soon, with the first data release scheduled for 2016. This review discusses the current state of our understanding of the kinematics of star formation and how the community can best prepare for Gaia data
The Gaia-ESO Survey (GES) observed many open clusters as part of its programme to spectroscopically ...
We live in a new era in Astrophysics driven by the launch of the European satellite Gaia. Gaia is cu...
We present the first large-scale 3D kinematic study of ~2000 spectroscopically-confirmed young stars...
The GAIA astrometric satellite will measure positions, proper motions and parallaxes of millions of ...
The GAIA astrometric mission has recently been approved as one of thenext two ``cornerstones'' of ES...
The Gaia mission has opened a new window into the internal kinematics of young star clusters at the ...
ESA’s Gaia mission will provide accurate astrometric, photometric and spectroscopic data for million...
The census of stellar structures and star clusters in the Milky Way has been vastly improved in the ...
ESA's Gaia mission will provide accurate astrometric, photometric andspectroscopic data for millions...
Gaia is an all sky, high precision astrometric and photometric satellite of the European Space Agenc...
Gaia is a fully-approved all-sky astrometric and photometric survey due for launch in 2011. It will ...
Star formation is a current relevant and active field that involves a wide range of physical process...
Identifying and characterizing young populations of star-forming regions are crucial to unraveling t...
In this thesis we study the kinematics and dynamics of our Galaxy, the Milky Way. We use data from t...
Stellar kinematics provides the key to understanding the formation process and dynamical evolution o...
The Gaia-ESO Survey (GES) observed many open clusters as part of its programme to spectroscopically ...
We live in a new era in Astrophysics driven by the launch of the European satellite Gaia. Gaia is cu...
We present the first large-scale 3D kinematic study of ~2000 spectroscopically-confirmed young stars...
The GAIA astrometric satellite will measure positions, proper motions and parallaxes of millions of ...
The GAIA astrometric mission has recently been approved as one of thenext two ``cornerstones'' of ES...
The Gaia mission has opened a new window into the internal kinematics of young star clusters at the ...
ESA’s Gaia mission will provide accurate astrometric, photometric and spectroscopic data for million...
The census of stellar structures and star clusters in the Milky Way has been vastly improved in the ...
ESA's Gaia mission will provide accurate astrometric, photometric andspectroscopic data for millions...
Gaia is an all sky, high precision astrometric and photometric satellite of the European Space Agenc...
Gaia is a fully-approved all-sky astrometric and photometric survey due for launch in 2011. It will ...
Star formation is a current relevant and active field that involves a wide range of physical process...
Identifying and characterizing young populations of star-forming regions are crucial to unraveling t...
In this thesis we study the kinematics and dynamics of our Galaxy, the Milky Way. We use data from t...
Stellar kinematics provides the key to understanding the formation process and dynamical evolution o...
The Gaia-ESO Survey (GES) observed many open clusters as part of its programme to spectroscopically ...
We live in a new era in Astrophysics driven by the launch of the European satellite Gaia. Gaia is cu...
We present the first large-scale 3D kinematic study of ~2000 spectroscopically-confirmed young stars...