activity
19962026
most citedFirst evidence of a magnetic field on Vega. Towards a new class of magnetic A-type stars

131 citations · 405 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

Fundamental properties of two rapidly rotating stars: Rasalhague and Alkaid

Axel Lazzarotto, Alain Hui-Bon-Hoa, Torsten Boehm +2

Abridged : The fundamental parameters of rapidly rotating stars are key quantities to understand the impact of rotation on stellar evolution. A few nearby early-type stars offer th…

astro-ph.SR2022★ 7 cited

Spectroscopic detection of Altair's non-radial pulsations

M. Rieutord, P. Petit, D. Reese +4

Context: Rapid rotation is a common feature of early-type stars but which remains a challenge for the models. The understanding of its effect on stellar evolution is however impera…

astro-ph.SR2022★ 9 cited

A decade-long magnetic monitoring of Vega

P. Petit, T. Böhm, C. P. Folsom +2

Aims. The very weak magnetic field detected at the surface of Vega hints at a widespread population of weakly magnetic stars of A and B spectral types. We contribute here to gather…

astro-ph.SR2016★ 59 cited

Detection of ultra-weak magnetic fields in Am stars: beta UMa and theta Leo

A. Blazère, P. Petit, F. Lignières +9

An extremely weak circularly polarized signature was recently discovered in spectral lines of the chemically peculiar Am star Sirius A. A weak surface magnetic field was proposed t…

astro-ph.EP2015★ 21 cited

A maximum entropy approach to detect close-in giant planets around active stars

P. Petit, J. -F. Donati, E. Hébrard +11

(shortened for arXiv) We aim to progress towards more efficient exoplanet detection around active stars by optimizing the use of Doppler Imaging in radial velocity measurements. We…

astro-ph.SR2011★ 8 cited

First evidence of pulsations in Vega? Results of today's most extensive spectroscopic search

Torsten Böhm, François Lignières, Gregg Wade +5

The impact of rapid rotation on stellar evolution theory remains poorly understood as of today. Vega is a special object in this context as spectroscopic and interferometric studie…

astro-ph.SR2010★ 93 cited

The rapid rotation and complex magnetic field geometry of Vega

P. Petit, F. Lignières, G. A. Wade +9

The recent discovery of a weak surface magnetic field on the normal intermediate-mass star Vega raises the question of the origin of this magnetism in a class of stars that was not…

astro-ph.SR2009★ 131 cited

First evidence of a magnetic field on Vega. Towards a new class of magnetic A-type stars

F. Lignieres, P. Petit, T. Bohm +1

We report the detection of a magnetic field on Vega through spectropolarimetric observations. We acquired 257 Stokes V, high signal-to-noise and high-resolution echelle spectra dur…

astro-ph2007

How non-magnetic are "non-magnetic" Herbig Ae/Be stars?

G. A. Wade, E. Alecian, C. Catala +9

Our recent discovery of magnetic fields in a small number of Herbig Ae/Be stars has required that we survey a much larger sample of stars. From our FORS1 and ESPaDOnS surveys, we h…

astro-ph1996★ 77 cited

Line profile variations in Doradus

L. A. Balona, T. Böhm, B. H. Foing +11

We present data from high-dispersion echelle spectra and simultaneous photometry for ~Doradus. These data were obtained from several sites during 1994 November as part of…