![Present-day and Early Star Formation](https://support.digitalhusky.com/media/annotations/sorted/451/4519434/CHSBZCOP034519434.jpg)
Present-day and Early Star Formation
Stars form from molecular cloud cores by gravoturbulent fragmentation. Understanding the angular momentum and the thermal evolution of cloud cores thus plays a fundamental role in completing the theoretical picture of star formation. This is true not only for current star formation as observed in regions like the Orion nebula or the ¿-Ophiuchi molecular cloud but also for the formation ...