Water In Star forming regins with Herschel
The Water In Star forming regions with Herschel (WISH) program was a guaranteed time key program with Herschel, led by Ewine van Dishoeck. Within the framework of this program, water was observed towards a large sample of protostars. These sources covered a wide range of masses, and a large range of evolutionary stages. I was part of the WISH outflow team, where we mapped the water emission towards a sample of outflows. A larger number of sources were targeted with pointed observations.
Selected publications
- Resolving the shocked gas in HH 54 with Herschel. CO line mapping at high spatial and spectral resolution
- First spectrally-resolved H2 observations towards HH 54 . Low H2O abundance in shocks
- Physical properties of outflows: Comparing CO- and H2O- based parameters in Class 0 sources
- Water in molecular outflows and shocks: Studies with Odin and Herschel
- H2O line mapping at high spatial and spectral resolution. Herschel observations of the VLA 1623 outflow
- Herschel observations of the Herbig-Haro objects HH 52-54
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