output
19922026
Showing 2014 · astro-ph.EPShow all

17 papers · 2 filters

astro-ph.EP2014★ 256 cited

Shadows cast by a warp in the HD 142527 protoplanetary disk

Sebastian Marino, Sebastian Perez, Simon Casassus

Detailed observations of gaps in protoplanetary disks have revealed structures that drive current research on circumstellar disks. One such feature is the two intensity nulls seen…

astro-ph.EP2014★ 91 cited

The HARPS search for southern extra-solar planets XXXV. Planetary systems and stellar activity of the M dwarfs GJ 3293, GJ 3341, and GJ 3543

N. Astudillo-Defru, X. Bonfils, X. Delfosse +13

Context. Planetary companions of a fixed mass induce larger amplitude reflex motions around lower-mass stars, which helps make M dwarfs excellent targets for extra-solar planet sea…

astro-ph.EP2014★ 94 cited

CO gas inside the protoplanetary disk cavity in HD 142527: disk structure from ALMA

Sebastian Perez, S. Casassus, F. Ménard +6

Inner cavities and annular gaps in circumstellar disks are possible signposts of giant planet formation. The young star HD 142527 hosts a massive protoplanetary disk with a large c…

astro-ph.EP2014★ 37 cited

A planetary system and a highly eccentric brown dwarf around the giant stars HIP67851 and HIP97233

M. I. Jones, J. S. Jenkins, P. Rojo +2

Context: So far more than 60 substellar companions have been discovered around giant stars. These systems present physical and orbital properties that contrast to those detected or…

astro-ph.EP2014★ 41 cited

The Debris Disk of Solar Analogue Ceti: Herschel Observations and Dynamical Simulations of the Proposed Multiplanet System

S. M. Lawler, J. Di Francesco, G. M. Kennedy +16

Ceti is a nearby, mature G-type star very similar to our Sun, with a massive Kuiper Belt analogue (Greaves et al. 2004) and possible multiplanet system (Tuomi et al. 2013) that…

astro-ph.EP2014★ 1 cited

Binary frequency of planet-host stars at wide separations: A new brown dwarf companion to a planet-host star

N. Lodieu, A. Perez-Garrido, V. J. S. Bejar +5

The aim of the project is to improve our knowledge on the multiplicity of planet-host stars at wide physical separations. We cross-matched approximately 6200 square degree area of…