J
Jerome Bouvier
Researcher at University of Grenoble
Publications - 290
Citations - 15149
Jerome Bouvier is an academic researcher from University of Grenoble. The author has contributed to research in topics: Stars & T Tauri star. The author has an hindex of 70, co-authored 278 publications receiving 13724 citations. Previous affiliations of Jerome Bouvier include Joseph Fourier University & Centre national de la recherche scientifique.
Papers
More filters
Journal ArticleDOI
A Census of the Young Cluster IC 348
Kevin Luhman,John R. Stauffer,August Muench,George H. Rieke,Elizabeth A. Lada,Jerome Bouvier,Charles J. Lada +6 more
TL;DR: In this paper, a new census of the stellar and substellar members of the young cluster IC 348 is presented, which contains a total of 288 members, 23 of which are later than M6 and thus are likely to be brown dwarfs.
Journal ArticleDOI
Accretion Disks around T Tauri Stars
TL;DR: In this paper, a simple model consisting of an active PMS star and active accretion disk is considered to explain the spectral energy distributions of T Tauri stars from 0.2 to 10 microns.
Journal ArticleDOI
Improved angular momentum evolution model for solar-like stars
François Gallet,Jerome Bouvier +1 more
TL;DR: In this paper, the rotational evolution of solar-like stars between 1 Myr and 10 Gyr with the aim of reproducing the distributions of rotational periods observed for star forming regions and young open clusters within this age range was studied.
Journal ArticleDOI
Stellar magnetism: empirical trends with age and rotation
Aline A. Vidotto,Aline A. Vidotto,Scott G. Gregory,Moira Jardine,Jean-François Donati,Pascal Petit,Julien Morin,Colin P. Folsom,Jerome Bouvier,Andrew Collier Cameron,G. A. J. Hussain,Stephen C. Marsden,Ian A. Waite,Rim Fares,Sandra V. Jeffers,J. D. do Nascimento +15 more
TL;DR: In this article, the observed large-scale surface magnetic fields of low-mass stars were reconstructed through Zeeman-Doppler imaging (ZDI), and the results indicated that small and large scale fields could share the same dynamo field generation processes.
Journal ArticleDOI
CSI 2264: SIMULTANEOUS OPTICAL AND INFRARED LIGHT CURVES OF YOUNG DISK-BEARING STARS IN NGC 2264 WITH CoRoT and SPITZER—EVIDENCE FOR MULTIPLE ORIGINS OF VARIABILITY*
Ann Marie Cody,John R. Stauffer,Annie Baglin,Giuseppina Micela,Luisa Rebull,Ettore Flaccomio,Maria Morales-Calderon,Suzanne Aigrain,Jerome Bouvier,Lynne A. Hillenbrand,Robert A. Gutermuth,Inseok Song,Neal J. Turner,Silvia H. P. Alencar,Konstanze Zwintz,Peter Plavchan,John M. Carpenter,Krzysztof Findeisen,Sean Carey,Susan Terebey,Lee Hartmann,Nuria Calvet,Paula S. Teixeira,Frederick J. Vrba,Scott J. Wolk,Kevin R. Covey,Katja Poppenhaeger,Hans Moritz Günther,Jan Forbrich,Jan Forbrich,Barbara Whitney,Laura Affer,William Herbst,Joseph L. Hora,David Barrado,Jon Holtzman,Franck Marchis,Kenneth Wood,M. M. Guimarães,Jorge Lillo Box,Edward Gillen,Amy McQuillan,Catherine Espaillat,Lori Allen,Paola D'Alessio,Fabio Favata +45 more
TL;DR: The Coordinated Synoptic Investigation of NGC 2264 (CSI 2264) as discussed by the authors was a 30-day multi-wavelength photometric monitoring campaign on more than 1000 young star members using 16 telescopes.