Francesco Trotta YERAC, Manchester - 2011 Using mm observations to constrain variations of dust properties in circumstellar disks Advised by: Leonardo.
Rich cluster [M ~ 10 15 M sun ] Large groups (Small clusters) [M ~ 10 13 - 10 14 M sun ] Environmental effects on neutral and molecular hydrogen of galaxies.
Effects of Young Clusters on Forming Solar Systems
THE BIRTH OF STARS AND PLANETARY SYSTEMS
![Rich cluster [M ~ 10 15 M sun ] Large groups (Small clusters) [M ~ 10 13 - 10 14 M sun ] Environmental effects on neutral and molecular hydrogen of galaxies.](https://static.fdocuments.net/doc/330x215/56649d315503460f94a0a1da/rich-cluster-m-10-15-m-sun-large-groups-small-clusters-m-10-13-.jpg)
