activity
20032021
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 2.1k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.EP2021

The formation of planetary systems with SPICA

I. Kamp, M. Honda, H. Nomura +38

In this era of spatially resolved observations of planet forming disks with ALMA and large ground-based telescopes such as the VLT, Keck and Subaru, we still lack statistically rel…

astro-ph.GA2021★ 174 cited

Water in star-forming regions (WISH): Physics and chemistry from clouds to disks as probed by Herschel spectroscopy

E. F. van Dishoeck, L. E. Kristensen, the WISH team

(abridged) Data and results from the WISH key program are summarized, designed to provide a legacy data set to address its physics and chemistry. WISH targeted ~80 sources along th…

astro-ph.EP2019★ 6 cited

Upper limits on the water vapour content of the Pictoris debris disk

M. Cavallius, G. Cataldi, A. Brandeker +3

The debris disk surrounding ~Pictoris has been observed with ALMA to contain a belt of CO gas with a distinct peak at 85 au. This CO clump is thought to be the result of a…

astro-ph.IM2018★ 124 cited

SPICA - a large cryogenic infrared space telescope Unveiling the obscured Universe

P. R. Roelfsema, H. Shibai, L. Armus +66

Measurements in the infrared wavelength domain allow us to assess directly the physical state and energy balance of cool matter in space, thus enabling the detailed study of the va…

astro-ph.GA2017★ 18 cited

Gas and dust in the star-forming region rho Oph A: II. The gas in the PDR and in the dense cores

Bengt Larsson, Rene Liseau

We investigate to what degree local physical and chemical conditions are related to the evolutionary status of various objects in star-forming media. rho Oph A displays the entire…

astro-ph.GA2017

A CS survey of small molecular cores

Bengt Larsson, René Liseau

We are addressing the sites of isolated low mass star formation in the solar neighbourhood, i.e. small cloud cores within one kiloparsec. We aim at determining the physical paramet…