activity
19982026
most citedSpectral Line Selection for HMI: A Comparison of Fe I 6173 and Ni I 6768

129 citations · 685 across the 25 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2025★ 2 cited

Making sense of the spectral line profiles of Betelgeuse and other Red SuperGiants

A. López Ariste, Q. Pilate, A. Lavail +1

Spectropolarimetry of atomic lines in the spectra of Betelgeuse, and other Red SuperGiants (RSG), presents broad line profiles in linear polarization, but narrow profiles in intens…

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.SR2019★ 8 cited

Asymmetric shocks in Cyg observed with linear spectropolarimetry

A. López Ariste, B. Tessore, E. S. Carlín +7

Aims: From a coherent interpretation of the linear polarisation detected in the spectral lines of the Mira star Cyg, we derive information about the dynamics of the stellar pho…

astro-ph.SR2016★ 59 cited

The close circumstellar environment of Betelgeuse. IV. VLTI/PIONIER interferometric monitoring of the photosphere

M. Montargès, P. Kervella, G. Perrin +9

Context. The mass-loss mechanism of cool massive evolved stars is poorly understood. The proximity of Betelgeuse makes it an appealing target to study its atmosphere, map the shape…

astro-ph.SR2014★ 3 cited

Ultra weak magnetic fields in Am stars: Beta UMa and theta Leo

Aurore Blazère, Pascal Petit, François Lignières +3

An extremely weak circularly-polarized signature was recently discovered in spectral lines of the chemically peculiar Am star Sirius A (Petit et al. 2011). This signal was interpre…

astro-ph.SR2012★ 6 cited

Scales of the magnetic fields in the quiet Sun

A. López Ariste, A. Sainz Dalda

Context: The presence of a turbulent magnetic field in the quiet Sun has been unveiled observationally using different techniques. The magnetic field is quasi-isotropic and has fie…