activity
19982015
most citedThe MiMeS Survey of Magnetism in Massive Stars: Introduction and overview

232 citations · 361 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2015★ 232 cited

The MiMeS Survey of Magnetism in Massive Stars: Introduction and overview

G. A. Wade, C. Neiner, E. Alecian +47

The MiMeS project is a large-scale, high resolution, sensitive spectropolarimetric investigation of the magnetic properties of O and early B type stars. Initiated in 2008 and compl…

astro-ph.SR2010★ 18 cited

Photometric variability of the Be star CoRoT-ID 102761769

M. Emilio, L. Andrade, E. Janot-Pacheco +16

Classical Be stars are rapid rotators of spectral type late O to early A and luminosity class V-III, wich exhibit Balmer emission lines and often a near infrared excess originating…

astro-ph2008

The Gaia satellite: a tool for Emission Line Stars and Hot Stars

Christophe Martayan, Yves Fremat, Ronny Blomme +19

The Gaia satellite will be launched at the end of 2011. It will observe at least 1 billion stars, and among them several million emission line stars and hot stars. Gaia will provid…

astro-ph2007★ 94 cited

Discovery of new nearby L and late-M dwarfs at low Galactic latitude from the DENIS database

N. Phan-Bao, M. S. Bessell, E. L. Martin +9

We report new nearby L and late-M dwarfs (d_phot <= 30 pc) discovered in our search for nearby ultracool dwarfs (I-J >= 3.0, later than M8.0) at low Galactic latitude (|b| < 15 deg…

astro-ph2005★ 14 cited

Near-IR Surface Brightness Fluctuations and Optical Colours of Magellanic Star Clusters

Rosa A. Gonzalez-Lopezlira, Marna Y. Albarran, Mustapha Mouhcine +3

This work continues our efforts to calibrate model surface brightness luminosities for the study of unresolved stellar populations, through the comparison with data of Magellanic C…

astro-ph1998★ 3 cited

New Young Stellar Object candidates in the Chamaeleon I molecular cloud discovered by DENIS

L. Cambresy, E. Copet, N. Epchtein +5

This paper presents an analysis of the nature of point sources discovered by DENIS in an area of 1.5 x 3 degrees around the Chamaeleon I molecular cloud. Most of the 30000 objects…