Abstract
Most stars are not born in isolation, but in a cluster environment. This means that gravitational interactions might lead to chances in the disc properties. Numerically modelling the Orion Nebula Cluster, as an example, we investigate how the cluster environment influences through gravitational interactions disc properties like disc frequency, disc mass, angular momentum transport and accretion. We show that the massive stars in the cluster center are the engines driving these processes and that their discs are most effected.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.