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Sean M. Andrews

4 papers hereh-index 4149 citations5 works total

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

author position
  • middle author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP3
  • astro-ph.SR1
same name
  • Sean M. Andrews — 20 papers, h 3
  • Sean M. Andrews — 16 papers, h 4
  • Sean M. Andrews — 3 papers
  • Sean M. Andrews — 1 paper

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

activity
20122025
most citedCan grain growth explain transition disks?

134 citations · 179 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2025

Observational Constraints on Evolution of Dust Disc Properties in Upper Scorpius

Paola Pinilla, Anibal Sierra, Nicolas T. Kurtovic +8

Protoplanetary discs in the Upper Scorpius star-forming region are excellent laboratories to investigate late stages of planet formation. In this work, we analyse the morphology of…

astro-ph.EP2024★ 35 cited

Population Synthesis Models Indicate a Need for Early and Ubiquitous Disk Substructures

Luca Delussu, Tilman Birnstiel, Anna Miotello +3

Large mm surveys of star forming regions enable the study of entire populations of planet-forming disks and reveal correlations between their observable properties. Population stud…

astro-ph.EP2023★ 10 cited

Millimeter emission in photoevaporating disks is determined by early substructures

Matías Gárate, Til Birnstiel, Paola Pinilla +7

[abridged]Photoevaporation and dust-trapping are individually considered to be important mechanisms in the evolution and morphology of protoplanetary disks. We studied how the pres…

astro-ph.SR2012★ 134 cited

Can grain growth explain transition disks?

T. Birnstiel, S. M. Andrews, B. Ercolano

Aims: Grain growth has been suggested as one possible explanation for the diminished dust optical depths in the inner regions of protoplanetary "transition" disks. In this work, we…

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