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

80 citations · 305 across the 6 of their papers we have counts for

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6 papers

astro-ph.SR2010★ 35 cited

The β Pictoris disk imaged by Herschel PACS and SPIRE

B. Vandenbussche, B. Sibthorpe, B. Acke +40

We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V star β Pic. The disk is well resolved in the PACS filters at 70, 100, and 160 μ…

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.EP2010★ 62 cited

The Vega Debris Disc: A view from Herschel

B. Sibthorpe, B. Vandenbussche, J. S. Greaves +37

We present five band imaging of the Vega debris disc obtained using the Herschel Space Observatory. These data span a wavelength range of 70-500 um with full-width half-maximum ang…

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…