activity
19992020
most citedThe XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

372 citations · 2.7k across the 38 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.SR2016★ 7 cited

Investigating the rotational evolution of very low-mass stars and brown dwarfs in young clusters using Monte Carlo simulations

M. J. Vasconcelos, J. Bouvier

Context. Very low-mass (VLM) stars and brown dwarfs (BDs) present a different rotational behaviour from their solar mass counter-parts. Aims. We investigate the rotational evolutio…

astro-ph.SR2016★ 26 cited

A revised moving cluster distance to the Pleiades open cluster

P. A. B. Galli, E. Moraux, H. Bouy +3

Aims: We provide a new distance estimate for the Pleiades based on the moving cluster method, which will be useful to further discuss the so-called Pleiades distance controversy an…

astro-ph.SR2016★ 25 cited

The seven sisters DANCe.II. Proper motions and the lithium-rotation-activity connection for G and K Pleiads

D. Barrado, H. Bouy, J. Bouvier +7

Stellar clusters are open windows to understand stellar evolution. Specifically, the change with time and the dependence on mass of different stellar properties. As such, they are…

astro-ph.SR2016★ 84 cited

Rotation in the Pleiades with K2: II. Multi-Period Stars

L. M. Rebull, J. R. Stauffer, J. Bouvier +15

We use K2 to continue the exploration of the distribution of rotation periods in Pleiades that we began in Paper I. We have discovered complicated multi-period behavior in Pleiades…

astro-ph.SR2016★ 220 cited

Rotation in the Pleiades with K2: I. Data and First Results

L. M. Rebull, J. R. Stauffer, J. Bouvier +16

Young (125 Myr), populous (1000 members), and relatively nearby, the Pleiades has provided an anchor for stellar angular momentum models for both younger and older stars. We use…

astro-ph.SR2016★ 64 cited

The Gaia-ESO Survey: A lithium-rotation connection at 5 Myr?

J. Bouvier, A. Lanzafame, L. Venuti +37

We investigate here the lithium content of young low-mass stars in the 5~Myr-old star forming region NGC~2264 and its relationship with rotation. We combine lithium equivalent widt…