activity
19982024
most citedThe surprising magnetic topology of tauSco: fossil remnant or dynamo output?

496 citations · 1.7k across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.SR2024★ 10 cited

Investigation of the Nature of the B[e] Star CI Cam in the Optical Range

E. A. Barsukova, A. N. Burenkov, V. P. Goranskij +10

We report the results of 24 years of photometric and spectroscopic monitoring of CI Cam since its outburst in 1998. In the early years of our research, we identified a system compo…

astro-ph.SR2022★ 15 cited

Time-Variable Jet Ejections from RW Aur A, RY Tau and DG Tau

Michihiro Takami, Hans Moritz Guenther, P. Christian Schneider +17

We present Gemini-NIFS, VLT-SINFONI and Keck-OSIRIS observations of near-infrared [Fe II] emission associated with the well-studied jets from three active T Tauri stars; RW Aur A,…

astro-ph.SR2022★ 16 cited

First detection of a magnetic field in low-luminosity B[e] stars: New scenarios for the nature and evolutionary stages of FS CMa stars

D. Korcakova, F. Sestito, N. Manset +8

We report the first detection of the magnetic field in a star of FS CMa type, a subgroup of objects characterized by the B[e] phenomenon. The split of magnetically sensitive lines…

astro-ph.SR2020

Possible Time Correlation Between Jet Ejection and Mass Accretion for RW Aur A

Michihiro Takami, Tracy L. Beck, P. Christian Schneider +17

For the active T-Taur star RW Aur A we have performed long-term (~10 yr) monitoring observations of (1) jet imaging in the [Fe II] 1.644-micron emission line using Gemini-NIFS and…

astro-ph.SR2020★ 49 cited

Spin-orbit alignment and magnetic activity in the young planetary system AU Mic

E. Martioli, G. Hebrard, C. Moutou +21

We present high resolution near-infrared spectropolarimetric observations using the SPIRou instrument at CFHT during a transit of the recently detected young planet AU Mic b, with…

astro-ph.SR2020★ 18 cited

Properties of Galactic B[e] Supergiants: V. 3 Pup -- constraining the orbital parameters and modeling the circumstellar environments

A. S. Miroshnichenko, S. Danford, S. V. Zharikov +9

We report the results of a long-term spectroscopic monitoring of the A-type supergiant with the B[e] phenomenon 3 Pup = HD 62623. We confirm earlier findings that it is a binary sy…