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M. Sebastian

3 papers hereh-index 3130 citations21 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author2
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • physics.bio-ph1
same name
  • M. Sebastian — 1 paper, h 57
  • M. Sebastian — 1 paper, h 5

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators
Showing astro-ph.GAShow all

2 papers · 1 filter

astro-ph.GA2026

The Local Star Formation Environment Predicts Young Star Cluster Radii: Evidence from PHANGS-MUSE H-alpha Maps

Michelle Sebastian

The effective radii of young star clusters correlate with cluster mass, but the large scatter about that relation is not well understood. Theory predicts that a cluster's initial r…

astro-ph.GA2026

Influence of star cluster mass, age, and galaxy star formation rate on star cluster radii

Michelle Sebastian

Star clusters are key components of galaxies, and the relationship between cluster radius and mass encodes information about cluster formation and evolution. Theoretical models pre…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.