CORDIS Project
Funding breakdown and partner intelligence are Premium
Sign in and upgrade to Premium for EU contribution totals, consortium analytics, OpenAlex research context, and AI summaries. · 0 consortium intelligence fields visible of 1
Start free • Cancel anytime • 14-day refund guarantee
This project explores the formation of astrophysical jets in various celestial objects, focusing on Symbiotic Stars as a case study. By examining the relationship between mass loss and accretion rates, the research aims to uncover the mechanisms behind jet formation across different astronomical phenomena.
Although jets are ubiquitous phenomena in many different astrophysical objects, their formation is still relatively unclear.
We find jets in young stellar objects (YSO), in Planetary and Proto-Planetary nebulae, in Symbiotic Stars (SySs), in X-ray binaries and active galactic nuclei.
The mass loss rate of all jets is found to be connected to the mass accretion rate of the underlying disk found in most objects.
Hence it is believed that a single universal mechanism is responsible for ejecting jet…
UNIVERSITA DEGLI STUDI DI TORINO
Partner organizations (coordinator is shown above), with normalized type and CORDIS activity type. Guests see up to 4 partners.
Similar projects, consortium collaboration history, frequent partners, and OpenAlex research context.
Guests see up to 5 topics.
