Simulations show massive main-sequence stars can retain up to about 10% of their mass when jets remove their outer envelope, preventing runaway expansion.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Enabling high mass accretion rates onto massive main sequence stars by outer envelope mass removal
Simulations show massive main-sequence stars can retain up to about 10% of their mass when jets remove their outer envelope, preventing runaway expansion.