activity
20042025
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 6.2k across the 74 of their papers we have counts for

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Showing 2018Show all

10 papers · 1 filter

astro-ph.GA2018★ 28 cited

Feedback in W49A diagnosed with radio recombination lines and models

M. R. Rugel, D. Rahner, H. Beuther +20

We present images of radio recombination lines (RRLs) at wavelengths around 17 cm from the star-forming region W49A to determine the kinematics of ionized gas in the THOR survey (T…

astro-ph.SR2018★ 6 cited

Dynamical masses of M-dwarf binaries in young moving groups: II - Toward empirical mass-luminosity isochrones

Markus Janson, Stephen Durkan, Mickael Bonnefoy +6

Low-mass stars exhibit substantial pre-main sequence evolution during the first ~100 Myrs of their lives. Thus, young M-type stars are prime targets for isochronal dating, especial…

astro-ph.EP2018★ 81 cited

Multiple water band detections in the CARMENES near-infrared transmission spectrum of HD 189733 b

F. J. Alonso-Floriano, A. Sánchez-López, I. A. G. Snellen +27

Aims: We explore the capabilities of CARMENES for characterizing hot-Jupiter atmospheres by targeting multiple water bands, in particular, those at 1.15 and 1.4 m. Hubble Space…

astro-ph.IM2018★ 54 cited

Origin of the asymmetry of the wind driven halo observed in high contrast images

F. Cantalloube, E Por, K. Dohlen +9

The latest generation of high contrast instruments dedicated to exoplanets and circumstellar disks imaging are equipped with extreme adaptive optics and coronagraphs to reach contr…

astro-ph.GA2018★ 46 cited

SEDIGISM: The kinematics of ATLASGAL filaments

M. Mattern, J. Kauffmann, T. Csengeri +13

Analysing the kinematics of filamentary molecular clouds is a crucial step towards understanding their role in the star formation process. Therefore, we study the kinematics of 283…

astro-ph.SR2018★ 20 cited

Dynamical masses of M-dwarf binaries in young moving groups: I - The case of TWA 22 and GJ 2060

L. Rodet, M. Bonnefoy, S. Durkan +48

Evolutionary models are widely used to infer the mass of stars, brown dwarfs, and giant planets. Their predictions are thought to be less reliable at young ages ( 200 Myr) and i…