activity
20022019
most citedA giant exoplanet orbiting a very low-mass star challenges planet formation models

130 citations · 486 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.EP2019★ 130 cited

A giant exoplanet orbiting a very low-mass star challenges planet formation models

J. C. Morales, A. J. Mustill, I. Ribas +179

Statistical analyses from exoplanet surveys around low-mass stars indicate that super-Earth and Neptune-mass planets are more frequent than gas giants around such stars, in agreeme…

astro-ph.SR2015★ 4 cited

Spectroscopic variability of two Oe stars

G. Rauw, T. Morel, Y. Naze +28

The Oe stars HD45314 and HD60848 have recently been found to exhibit very different X-ray properties: whilst HD60848 has an X-ray spectrum and emission level typical of most OB sta…

astro-ph.SR2014★ 9 cited

The variable stellar wind of Rigel probed at high spatial and spectral resolution

O. Chesneau, A. Kaufer, O. Stahl +5

We present a spatially resolved, high-spectral resolution (R=12000) K-band temporal monitoring of Rigel using AMBER at the VLTI. Rigel was observed in the Bracket Gamma line and it…

astro-ph.SR2013★ 29 cited

Broad-band Spectroscopy of the Ongoing Large Eruption of the Luminous Blue Variable R71

A. Mehner, D. Baade, T. Rivinius +4

The Luminous Blue Variable (LBV) R71 is currently undergoing an eruption, which differs photometrically and spectroscopically from its last outburst in the 1970s. Valuable informat…

astro-ph.GA2012★ 7 cited

Is there a compact companion orbiting the late O-type binary star HD 164816?

L. Trepl, V. V. Hambaryan, T. Pribulla +7

We present a multi-wavelength (X-ray, -ray, optical and radio) study of HD 194816, a late O-type X-ray detected spectroscopic binary. X-ray spectra are analyzed and the X-ray ph…

astro-ph.SR2011

The WR 140 periastron passage 2009: first results from MONS and other optical sources

R. Fahed, A. F. J. Moffat, J. Zorec +29

We present the results from the spectroscopic follow-up of WR140 (WC7 + O4-5) during its last periastron passage in January 2009. This object is known as the archetype of colliding…