activity
20062014
most citedDiscovery of magnetic fields in the very young, massive stars W601 (NGC 6611) and OI 201 (NGC 2244)

44 citations · 66 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2014

PCA-based inversion of stellar fundamental parameters from high-resolution Echelle spectra

F. Paletou, J. -F. Trouilhet, T. Boehm

The general context of this study is the inversion of stellar fundamental parameters from high-resolution Echelle spectra. We aim at developing a fast and reliable tool for the pos…

astro-ph.SR2011★ 10 cited

Spectroscopic monitoring of the Herbig Ae star HD 104237. II. Non-radial pulsations, mode analysis and fundamental stellar parameters

Aurelie Fumel, Torsten Boehm

Herbig Ae/Be stars are intermediate-mass pre-main sequence (PMS) stars showing signs of intense activity and strong stellar winds, whose origin is not yet understood in the frame o…

astro-ph2008★ 5 cited

Magnetism in Herbig Ae/Be stars and the link to the Ap/Bp stars

E. Alecian, C. Catala, G. A. Wade +11

Among the A/B stars, about 5% host large-scale organised magnetic fields. These magnetic stars show also abundance anomalies in their spectra, and are therefore called the magnetic…

astro-ph2008★ 44 cited

Discovery of magnetic fields in the very young, massive stars W601 (NGC 6611) and OI 201 (NGC 2244)

E. Alecian, G. A. Wade, C. Catala +8

Context: Recent spectropolarimetric observations of Herbig Ae/Be stars have yielded new arguments in favour of a fossil origin for the magnetic fields of intermediate mass stars. A…

astro-ph2007★ 6 cited

Magnetism in pre-MS intermediate-mass stars and the fossil field hypothesis

E. Alecian, G. A. Wade, C. Catala +11

Today, one of the greatest challenges concerning the Ap/Bp stars is to understand the origin of their slow rotation and their magnetic fields. The favoured hypothesis for the latte…

astro-ph2007

Magnetism and rotation in Herbig Ae/Be stars

E. Alecian, G. A. Wade, C. Catala +8

Among the main sequence intermediate mass A and B stars, around 5% host large-scale organized magnetic fields. Most of these stars are very slow rotators compared to their non-magn…