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20032015
most citedAsymmetric features in the protoplanetary disk MWC758

318 citations · 504 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2015★ 318 cited

Asymmetric features in the protoplanetary disk MWC758

M. Benisty, A. Juhasz, A. Boccaletti +25

The study of dynamical processes in protoplanetary disks is essential to understand planet formation. In this context, transition disks are prime targets because they are at an adv…

astro-ph.SR2015★ 1 cited

Spectro-astrometry of LkCa 15 with X-Shooter: Searching for emission from LkCa 15b

E. T. Whelan, N. Huelamo, J. M. Alcala +5

Planet formation is one explanation for the partial clearing of dust observed in the disks of some T Tauri stars. Indeed studies using state-of-the-art high angular resolution tech…

astro-ph.SR2010★ 80 cited

Herschel-PACS observation of the 10 Myr old T Tauri disk TW Hya: Constraining the disk gas mass

W. F. Thi, G. Mathews, F. Ménard +49

Planets are formed in disks around young stars. With an age of ~10 Myr, TW Hya is one of the nearest T Tauri stars that is still surrounded by a relatively massive disk. In additio…

astro-ph.SR2010★ 48 cited

Gas in the protoplanetary disc of HD 169142: Herschel's view

G. Meeus, C. Pinte, P. Woitke +50

In an effort to simultaneously study the gas and dust components of the disc surrounding the young Herbig Ae star HD 169142, we present far-IR observations obtained with the PACS i…

astro-ph.SR2010★ 27 cited

The Herschel view of Gas in Protoplanetary Systems (GASPS). First comparisons with a large grid of models

C. Pinte, P. Woitke, F. Menard +49

The Herschel GASPS Key Program is a survey of the gas phase of protoplanetary discs, targeting 240 objects which cover a large range of ages, spectral types, and disc properties. T…

astro-ph2003★ 30 cited

Late B-type stars and their candidate companions resolved with Chandra

B. Stelzer, N. Huelamo, S. Hubrig +6

We present the first results from a series of Chandra observations carried out with the aim to examine the origin of X-ray emission in main-sequence late B-type stars. We use high…