Publication Date:
2020-06-16
Description:
The mass growth of protostars is a central element to the determination of fundamental stellar population properties such as the initial mass function. Constraining the accretion history of individual protostars is therefore an important aspect of star formation research. The goal of the study presented here is to determine whether high-mass (proto)stars gain their mass from a compact (
Print ISSN:
0035-8711
Electronic ISSN:
1365-2966
Topics:
Physics