Star-formation (III)
18 Maio 2020, 13:00 • Israel Matute
From the Hayashi line to the ZAMS
Protostar formation when adiabatic core reached. The role of the opacity generated by H-.
The Hayashi track. Protostar evolution into the Hayashi line and the constraints imposed by convection:
Marks a completely convective limit (stability/No-stability)
Detailed follow-up of the processes that drive the 1 M☉ star evolution from the Hayashi line to the Zero-Age-Main-Sequence (ZAMS)