activity
20162024
most citedKELT-17b: A hot-Jupiter transiting an A-star in a misaligned orbit detected with Doppler tomography

75 citations · 110 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR20243 cited

HD 34736: An intensely magnetised double-lined spectroscopic binary with rapidly-rotating chemically peculiar B-type components

E. Semenko, O. Kochukhov, Z. Mikulášek +21

We report the results of a comprehensive study of the spectroscopic binary (SB2) system HD 34736 hosting two chemically peculiar (CP) late B-type stars. Using new and archival obse…

astro-ph.SR2024

TESS observations of non-Be fast rotators

Yael Naze, Nikolay Britavskiy, Jonathan Labadie-Bartz

The variability of fast-rotating Oe/Be stars has been reported in detail in recent years. However, much less known about the behaviour of fast-rotating OB stars without known decre…

astro-ph.SR20243 cited

Magnetism in LAMOST CP stars observed by TESS

Keegan Thomson-Paressant, Coralie Neiner, Jonathan Labadie-Bartz

Context. A thousand new magnetic candidate CP stars have been identified with LAMOST, among which about 700 prime targets have rotational modulation determined from TESS. Aims. We…

astro-ph.SR2023

Optical Properties and Variability of the Be X-ray binary CPD -29 2176

Clarissa M. Pavao, Noel D. Richardson, Jonathan Labadie-Bartz +2

Be X-ray binaries (Be XRBs) are high-mass X-ray binaries, with a neutron star or black hole orbiting and accreting material from a non-supergiant B-star that is rotating at a near…

astro-ph.SR2023

A search for magnetic Scuti stars in Kepler hybrid candidates

K. Thomson-Paressant, C. Neiner, P. Lampens +4

Numerous candidate hybrid stars of type Scuti - Doradus have been identified with the Kepler satellite. However, many of them lie outside the theoretically expected instabi…

astro-ph.SR202310 cited

Extreme mass ratios and fast rotation in three massive binaries

Yael Naze, Nikolay Britavskiy, Gregor Rauw +2

The origin of rapid rotation in massive stars remains debated, although binary interactions are now often advocated as a cause. However, the broad and shallow lines in the spectra…