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)

Galaktisk astrofysik

Finansiering

Chalmers

Finansierar Chalmers deltagande under 2017–

Mer information

Senast uppdaterat

2019-10-30