Outputs (5)

The Age of Taurus: Environmental Effects on Disc Lifetimes (2015)
Journal Article
Rees, J. M., Wilson, T., Bell, C. P. M., Jeffries, R. D., & Naylor, T. (2015). The Age of Taurus: Environmental Effects on Disc Lifetimes. Proceedings of the International Astronomical Union, 10(S314), 205-206. https://doi.org/10.1017/s1743921315006286

Using semi-empirical isochrones, we find the age of the Taurus star-forming region to be 3-4 Myr. Comparing the disc fraction in Taurus to young massive clusters suggests discs survive longer in this low density environment. We also present a method... Read More about The Age of Taurus: Environmental Effects on Disc Lifetimes.

The Gaia-ESO Survey: N-body modelling of the Gamma Velorum cluster (2015)
Journal Article
Mapelli, M., Vallenari, A., Jeffries, R. D., Gavagnin, E., Cantat-Gaudin, T., Sacco, G. G., …Worley, C. C. (2015). The Gaia-ESO Survey: N-body modelling of the Gamma Velorum cluster. Astronomy & Astrophysics, 578, A35. https://doi.org/10.1051/0004-6361/201425514

The Gaia-ESO Survey has recently unveiled the complex kinematic signature of the Gamma Velorum cluster: this cluster is composed of two kinematically distinct populations (hereafter, population A and B), showing two different velocity dispersions and... Read More about The Gaia-ESO Survey: N-body modelling of the Gamma Velorum cluster.

Gaia-ESO Survey: Analysis of pre-main sequence stellar spectra (2015)
Journal Article
Lanzafame, A. C., Frasca, A., Damiani, F., Franciosini, E., Cottaar, M., Sousa, S. G., …Zaggia, S. (2015). Gaia-ESO Survey: Analysis of pre-main sequence stellar spectra. Astronomy & Astrophysics, 576, Article A80. https://doi.org/10.1051/0004-6361/201424759

Context. The Gaia-ESO Public Spectroscopic Survey is obtaining high-quality spectroscopy of some 100 000 Milky Way stars using the FLAMES spectrograph at the VLT, down to V = 19 mag, systematically covering all the main components of the Milky Way an... Read More about Gaia-ESO Survey: Analysis of pre-main sequence stellar spectra.

TheGaia-ESO Survey: Chromospheric emission, accretion properties, and rotation inγVelorum and Chamaeleon I (2015)
Journal Article
Frasca, A., Biazzo, K., Lanzafame, A. C., Alcalá, J. M., Brugaletta, E., Klutsch, A., …Worley, C. C. (2015). TheGaia-ESO Survey: Chromospheric emission, accretion properties, and rotation inγVelorum and Chamaeleon I. Astronomy & Astrophysics, 575, A4. https://doi.org/10.1051/0004-6361/201424409

Aims. One of the goals of the Gaia-ESO Survey (GES), which is conducted with FLAMES at the VLT, is the census and the characterization of the low-mass members of very young clusters and associations. We conduct a comparative study of the main propert... Read More about TheGaia-ESO Survey: Chromospheric emission, accretion properties, and rotation inγVelorum and Chamaeleon I.

The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters (2015)
Journal Article
Lardo, C., Pancino, E., Bellazzini, M., Bragaglia, A., Donati, P., Gilmore, G., …Worley, C. C. (2015). The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters. Astronomy & Astrophysics, 573, Article A115. https://doi.org/10.1051/0004-6361/201425036

The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and formation history of our Galaxy by collecting spectroscopy of representative samples (about 105 Milky Way stars) of all Galactic stellar populations, in... Read More about The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters.