E. A. Bergin

TL;DR: Water In Star-forming regions with Herschel (WISH) as discussed by the authors is a key program on the Herschel Space Observatory designed to probe the physical and chemical structures of young stellar objects using water and related molecules and to follow the water abundance from collapsing clouds to planet-forming disks.

TL;DR: Water In Star-forming regions with Herschel (WISH) as mentioned in this paper is a key program on the Herschel Space Observatory designed to probe the physical and chemical structure of young stellar objects using water and related molecules and to follow the water abundance from collapsing clouds to planet-forming disks.

TL;DR: In this paper, the authors present a Herschel Space Observatory survey of six additional T T Tauri disks in the HD J = 1-0 line at 112 µm and establish upper limits to the line flux for the other four disks, using detailed disk structure and ray-tracing models.

TL;DR: In this article, the authors quantify the far-infrared line emission from low-mass protostars and the contribution of different atomic and molecular species to the gas cooling budget, to determine the spatial extent of the emission, and to investigate the underlying excitation conditions.

TL;DR: In this paper, the spectral properties of the Orion hot core were investigated using the Herschel GT key program and the HIFI spectra of Orion KL between 480 and 560 GHz and from 1.06 to 1.115 THz.