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researcher

S. Marino

61 papers hereh-index 241.7k citations74 works total

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

author position
  • sole author1
  • first author7
  • middle author43
  • last author4

Across the 55 of 61 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP52
  • astro-ph.SR6
  • astro-ph.GA2
  • astro-ph.HE1
same name
  • S. Marino — 13 papers, h 6
  • S. Marino — 11 papers, h 4
  • S. Marino — 6 papers, h 1
  • S. Marino — 1 paper, h 24
  • S. Marino — 1 paper, h 4
  • S. Marino — 1 paper, h 2

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
20152025
most citedCircumbinary, not transitional: On the spiral arms, cavity, shadows, fast radial flows, streamers and horseshoe in the HD142527 disc

186 citations · 2.6k across the 61 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

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.EP2025

Follow-Up Exploration of the TWA 7 Planet-Disk System with JWST NIRCam

Katie A. Crotts, Aarynn L. Carter, Kellen Lawson +39

The young M-star TWA 7 hosts a bright and near face-on debris disk, which has been imaged from the optical to the submillimeter. The disk displays multiple complex substructures su…

astro-ph.EP2025★ 2 cited

HD 143006: Interferometric Confirmation of Misaligned Protoplanetary Disc with CHARA/MIRCX and VLTI/PIONIER

I. Codron, S. Kraus, J. D. Monnier +7

The outer regions of the protoplanetary disc surrounding the T Tauri star HD 143006 show rings, dust asymmetries and shadows. Whilst rings and dust asymmetries can arise from compa…

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