A spiral pattern in the stellar velocity dispersion map of NGC 4030 correlates with star-forming regions, supporting the idea that stars inherit the motion of their parent gas and are later heated.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Large-Scale Stellar Age-Velocity Spiral Pattern in NGC 4030
A spiral pattern in the stellar velocity dispersion map of NGC 4030 correlates with star-forming regions, supporting the idea that stars inherit the motion of their parent gas and are later heated.