activity
20102019
most citedAn icy Kuiper-Belt around the young solar-type star HD 181327

123 citations · 333 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2019★ 2 cited

A Great Successor to the Hubble Space Telescope

B. Scott Gaudi, John C. Clarke, Shawn Domagal-Goldman +7

The Hubble Space Telescope (HST) has been the most impactful science-driven mission ever flown by NASA. However, when HST reaches the end of its life, there will be a void due to t…

astro-ph.EP2011★ 123 cited

An icy Kuiper-Belt around the young solar-type star HD 181327

J. Lebreton, J. -C. Augereau, W. -F. Thi +18

HD 181327 is a young F5/F6V star belonging to the Beta Pictoris moving group (12 Myr). It harbors an optically thin belt of circumstellar material at 90 AU. We aim to study the dus…

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-ph.SR2010★ 53 cited

Resolving the cold debris disc around a planet-hosting star: PACS photometric imaging observations of q1 Eri (HD10647, HR506)

R. Liseau, C. Eiroa, D. Fedele +32

About two dozen exo-solar debris systems have been spatially resolved. These debris discs commonly display a variety of structural features such as clumps, rings, belts, eccentric…