Star-forming regions in spiral arms and rings are often regularly spaced at 350 to 500 parsecs or multiples, a scale smaller than classical disk-instability predictions, with NGC 3627 added to the sample.
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
-
Regular distribution of star formation regions along the spiral arms and rings of disk galaxies
Star-forming regions in spiral arms and rings are often regularly spaced at 350 to 500 parsecs or multiples, a scale smaller than classical disk-instability predictions, with NGC 3627 added to the sample.