activity
20002020
most citedSearch for surface magnetic fields in Mira stars. First detection in chi Cyg

55 citations · 237 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2020

Pulsating chromosphere of classical Cepheids. Calcium infrared triplet and H profile variations

V. Hocdé, N. Nardetto, S. Borgniet +10

It has been shown recently that the infrared emission of Cepheids, which is constant over the pulsation cycle, might be due to a pulsating shell of ionized gas of about 15\% of the…

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.SR2019★ 18 cited

Dynamical structure of the pulsating atmosphere of RR Lyr - I. A typical pulsation cycle

D. Gillet, B. Mauclaire, T. Lemoult +5

RRab stars are large amplitude pulsating stars in which the pulsation is associated with strong shock wake propagating in the atmosphere. The objective of this study is to provide…

astro-ph.SR2017★ 9 cited

First observation of H redshifted emission in RR Lyr

D. Gillet, B. Mauclaire, T. Garrel +10

The so-called H third emission occurs around pulsation phase =0.30. It has been observed for the first time in 2011 in some RR Lyrae stars. The emission intensity is very wea…

astro-ph.IM2014★ 19 cited

An 8-mm diameter Fiber Robot Positioner for Massive Spectroscopy Surveys

N. Fahim, F. Prada, J. P. Kneib +22

Massive spectroscopic survey are becoming trendy in astrophysics and cosmology, as they can address new fundamental knowledge such as Galactic Archaeology and probe the nature of t…

astro-ph.SR2013★ 55 cited

Search for surface magnetic fields in Mira stars. First detection in chi Cyg

A. Lèbre, M. Aurière, N. Fabas +4

In order to complete the knowledge of the magnetic field and of its influence during the transition from Asymptotic Giant Branch to Planetary Nebulae stages, we have undertaken a s…