NASA NTRS · 19690041399
Dynamical stability in pre-main-sequence stars.
Abstract
Dynamical stability in premain sequence stars, discussing adiabatic models for pure hydrogen composition and collapse initiation by low opacity
Keep this discovery
Explore connections, maps & timelines
Dworetsky, M. M., Little, S. J., Upton, E. K. L.. 1968-11-01. Dynamical stability in pre-main-sequence stars.. https://ntrs.nasa.gov/citations/19690041399
Cite the original work for its findings. Save a collection to share your selection of sources.