PILS-Cygnus is a survey with the SMA of star formation in the Cygnus X region. Its main aim is to study the complex chemistry in low-mass hot corinos and intermediate mass hot cores, enabling the study of key chemical processes, molecular abundances, and shedding light on the fundamental chemistry in a statistically meaningful way.
Team members: Lars Kristensen (PI), Hannah Calcutt, Charl van der Walt, Jes Jørgensen, Manar el Akel, Karin Öberg, Keping Qiu, Robin Garrod, Joseph Mottram
Hannah Calcutt (contact)
Visiting Researcher at Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics, Galactic Astrophysics
Funding Chalmers participation during 2017–