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researcher

D. Romano

4 papers hereh-index 220 citations7 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.GA2
  • astro-ph.SR2
same name
  • D. Romano — 11 papers, h 9
  • D. Romano — 4 papers, h 1
  • D. Romano — 3 papers, h 1
  • D. Romano — 2 papers, h 6
  • D. Romano — 1 paper, h 3
  • D. Romano — 1 paper, h 33

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

Lithium evolution in the Galactic thin disc from Main-Sequence and early Red-Giant-Branch stars

C. T. Nguyen, G. Cescutti, F. Matteucci +7

The role of novae as producers of galactic lithium has been suggested since the 1970s, and it has been reconsidered recently with the detection of 7Be in their outbursts. At the…

astro-ph.SR2025

Probing the origins. II. Unravelling lithium depletion and stellar motion: Intrinsic stellar properties drive depletion, not kinematics

M. L. L. Dantas, R. Smiljanic, D. Romano +4

In Paper I, we classified a stellar sample from the thin disc with a broad range in metallicity as being churned outward or inward, or blurred/undisturbed. In this paper (Paper II)…

astro-ph.GA2025

The Bulge Cluster Origin (BulCO) survey at the ESO-VLT: probing the early history of the Milky Way assembling. Design and first results in Liller1

F. R. Ferraro, L. Chiappino, A. Bartolomei +14

We present the scientific goals and the very first results of the Bulge Cluster Origin (BulCO) survey. This survey has been specifically designed to perform an unprecedented chemic…

astro-ph.SR2025

The interplay between super-metallicity, lithium depletion, and radial migration in nearby stars

M. L. L. Dantas, R. Smiljanic, R. Boesso +4

We report the discovery of a peculiar set of old super-metal-rich dwarf stars with orbits of low eccentricity that reach a maximum height from the Galactic plane between ∼ 0.5…

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