activity
20162026
most citedSPIRou: nIR velocimetry & spectropolarimetry at the CFHT

172 citations · 1k across the 56 of their papers we have counts for

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14 papers · 1 filter

astro-ph.SR2026

Eta Carinae's historical light curve: evidence for cyclic Roche lobe overflow from the primary star

Augusto Damineli, Leonardo A. Almeida, Francisco J. Jablonski +5

The large amount of ground-based photometric measurements of Carinae obtained since 1940 have remained problematic for quantitative modeling due to the blending of flux from th…

astro-ph.SR2025

Extreme Lithium Depletion in Solar Twins: Challenging Non-Standard Mixing Models

Isabelle Winnick, Jhon Yana Galarza, Henrique Reggiani +12

Lithium (Li) is a powerful tracer of stellar mixing, gradually depleted in solar twins by non-standard transport below the convective zone. Here, we identify six new solar twins wi…

astro-ph.SR2024

HIP 8522: A Puzzling Young Solar Twin with the Lowest Detected Lithium

Jhon Yana Galarza, Diego Lorenzo-Oliveira, Thiago Ferreira +8

We present HIP 8522, a young solar twin with the lowest detected lithium, potentially a field blue straggler or the result of episodic early accretion. Its stellar parameters ($T_{…

astro-ph.SR2024

BEBOP V. Homogeneous Stellar Analysis of Potential Circumbinary Planet Hosts

Alix V. Freckelton, Daniel Sebastian, Annelies Mortier +29

Planets orbiting binary systems are relatively unexplored compared to those around single stars. Detections of circumbinary planets and planetary systems offer a first detailed vie…

astro-ph.SR2024

Long-term monitoring of large-scale magnetic fields across optical and near-infrared domains with ESPaDOnS, Narval and SPIRou. The cases of EV Lac, DS Leo, and CN Leo

S. Bellotti, J. Morin, L. T. Lehmann +18

Dynamo models of stellar magnetic fields for partly and fully convective stars are guided by observational constraints. Zeeman-Doppler imaging has revealed a variety of magnetic fi…

astro-ph.SR2024

Long period modulation of the classical T Tauri star CI Tau: evidence for an eccentric close-in massive planet at 0.17 au

R. Manick, A. P. Sousa, J. Bouvier +13

Detecting planets within protoplanetary disks around young stars is essential for understanding planet formation and evolution. However, planet detection using the radial velocity…