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researcher

L. Romano

4 papers hereh-index 326 citations8 works total

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

author position
  • first author1
  • middle author3

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

fields
  • astro-ph.GA4
same name
  • L. Romano — 3 papers, h 11
  • L. Romano — 3 papers, h 3
  • L. Romano — 1 paper, h 1
  • L. Romano — 1 paper, h 7
  • L. Romano — 1 paper, h 26

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

4 papers

astro-ph.GA2025

Cosmic Rays in Galaxy Halos: Impacts on Galactic Outflows and Baryon Cycling

Ellis R. Owen, Leonard E. C. Romano, Kentaro Nagamine

Galaxies with high star-formation rate surface densities often host large-scale outflows that redistribute energy, momentum, and baryons between the interstellar medium and the hal…

astro-ph.GA2025

Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions

Kosei Matsumoto, Laura Sommovigo, Andrea Gebek +8

We investigate the impacts of the evolution of dust mass and grain size distribution within a Milky Way-like (MW-like) galaxy simulation on global attenuation curves, focusing on t…

astro-ph.GA2025

Starburst-Driven Galactic Outflows -- Unveiling the Suppressive Role of Cosmic Ray Halos

Leonard E. C. Romano, Ellis R. Owen, Kentaro Nagamine

Aims. We investigate the role of cosmic ray (CR) halos in shaping the properties of starburst-driven galactic outflows. Methods. We develop a microphysical model for galactic outfl…

astro-ph.GA2024

Radial properties of dust in galaxies: Comparison between observations and isolated galaxy simulations

S. A. van der Giessen, K. Matsumoto, M. Relano +8

We study the importance of several processes that influence the evolution of dust and its grain size distribution on spatially resolved scales in nearby galaxies. Here, we compiled…

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