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Gaia view of low-mass star formation

Published online by Cambridge University Press:  07 March 2018

C. F. Manara Open the ORCID record for C. F. Manara [Opens in a new window] ,
T. Prusti ,
J. Voirin  and
E. Zari
C. F. Manara
Affiliation:
Scientific Support Office, Directorate of Science, European Space Research and Technology Centre (ESA/ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands email: [email protected]
T. Prusti
Affiliation:
Scientific Support Office, Directorate of Science, European Space Research and Technology Centre (ESA/ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands email: [email protected]
J. Voirin
Affiliation:
Scientific Support Office, Directorate of Science, European Space Research and Technology Centre (ESA/ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands email: [email protected]
E. Zari
Affiliation:
Leiden Observatory, Niels Bohrweg 2, 2333 CA Leiden, the Netherlands
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Abstract

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Understanding how young stars and their circumstellar disks form and evolve is key to explain how planets form. The evolution of the star and the disk is regulated by different processes, both internal to the system or related to their environment. The former include accretion of material onto the central star, wind emission, and photoevaporation of the disk due to high-energy radiation from the central star. These are best studied spectroscopically, and the distance to the star is a key parameter in all these studies. Here we present new estimates of the distance to a complex of nearby star-forming clouds obtained combining TGAS distances with measurement of extinction on the line of sight. Furthermore, we show how we plan to study the effects of the environment on the evolution of disks with Gaia, using a kinematic modelling code we have developed to model young star-forming regions.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 309 - 312
Copyright
Copyright © International Astronomical Union 2018 

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