output
20022024
most citedThe Gaia mission

7.1k citations

Showing 2013Show all

7 papers · 1 filter

astro-ph.EP201315 cited

A sensitivity analysis of the WFCAM Transit Survey for short-period giant planets around M dwarfs

Gábor Kovács, S. Hodgkin, B. Sipőcz +11

The WFCAM Transit Survey (WTS) is a near-infrared transit survey running on the United Kingdom Infrared Telescope (UKIRT), designed to discover planets around M dwarfs. The WTS act…

astro-ph.CO2013134 cited

The Lyman alpha Reference Sample: Extended Lyman alpha Halos Produced at Low Dust Content

Matthew Hayes, Göran Östlin, Daniel Schaerer +14

We report on new imaging observations of the Lyman alpha emission line (Lya), performed with the Hubble Space Telescope, that comprise the backbone of the Lyman alpha Reference Sam…

astro-ph.SR201336 cited

Proper motions of young stars in Chamaeleon. I. A Virtual Observatory study of spectroscopically confirmed members

Belén López Martí, Francisco Jiménez-Esteban, Amelia Bayo +3

(abridged) We want to provide further evidence of the origin of the proposed stellar members of Chamaeleon and to identify interlopers from the foreground εCha and ηCha association…

physics.chem-ph201325 cited

Spontaneous Mirror Symmetry Breaking in the Limited Enantioselective Autocatalysis Model: Abyssal Hydrothermal Vents as Scenario for the Emergence of Chirality in Prebiotic Chemistry

Josep M. Ribó, Joaquim Crusats, Zoubir El-Hachemi +3

The emergence of chirality in enantioselective autocatalysis for compounds unable to transform according to the Frank-like reaction network is discussed with respect to the controv…

astro-ph.GA2013108 cited

Low velocity shocks: signatures of turbulent dissipation in diffuse irradiated gas

Pierre Lesaffre, Guillaume Pineau des Forêts, Benjamin Godard +3

We examine the chemical and emission properties of mildly irradiated (G0=1) magnetised shocks in diffuse media (nH=10^2 to 10^4 /cm3) at low to moderate velocities (from 3 to 40 km…

astro-ph.GA2013109 cited

The chemistry of ions in the Orion Bar I. - CH+, SH+, and CF+: The effect of high electron density and vibrationally excited H2 in a warm PDR surface

Z. Nagy, F. F. S. Van der Tak, V. Ossenkopf +8

The abundances of interstellar CH+ and SH+ are not well understood as their most likely formation channels are highly endothermic. Using data from Herschel, we study the formation…