PILS-Cygnus
Forskningsprojekt , 2017 –

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

Deltagare

Hannah Calcutt (kontakt)

Doktor vid Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Galaktisk astrofysik

Finansiering

Chalmers

Finansierar Chalmers deltagande under 2017–

Mer information

Senast uppdaterat

2019-10-30