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researcher

P. Molaro

191 papers hereh-index 5117.3k citations444 works total

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

author position
  • sole author9
  • first author25
  • middle author109
  • last author26

Across the 169 of 191 papers where every author was matched, so the position is known.

fields
  • astro-ph73
  • astro-ph.EP38
  • astro-ph.CO28
  • astro-ph.SR20
  • astro-ph.GA14
  • astro-ph.IM12
same name
  • P. Molaro — 22 papers, h 6
  • P. Molaro — 20 papers, h 4
  • P. Molaro — 2 papers
  • P. Molaro — 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
19942025
most citedFirst stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy

1.2k citations · 9.9k across the 184 of their papers we have counts for

collaborators
Showing 2012Show all

4 papers · 1 filter

astro-ph.SR2012

Pre-MS depletion, accretion and primordial 7Li

P. Molaro, A. Bressan, M. Barbieri +2

We reconsider the role of pre-main sequence (pre-MS) Li depletion on the basis of new observational and theoretical evidence: i) new observations of Halpha emissions in young clust…

astro-ph.CO2012★ 45 cited

Deuterium at high-redshift: Primordial abundance in the zabs = 2.621 damped Ly-alpha system towards CTQ247

P. Noterdaeme, S. López, V. Dumont +3

The detection of neutral deuterium in the low-metallicity damped Lyman-α system at zabs = 2.621 towards the quasar CTQ247 is reported. Using a high signal-to-noise and high spectra…

astro-ph.CO2012★ 39 cited

QSO 0347-383 and the invariance of m_p/m_e in the course of cosmic time

Martin Wendt, Paolo Molaro

The variation of the dimensionless fundamental physical constant mu = m_p/m_e (the proton to electron mass ratio) can be constrained via observation of Lyman and Werner lines of mo…

astro-ph.GA2012★ 341 cited

An extremely primitive halo star

E. Caffau, P. Bonifacio, P. François +11

The early Universe had a chemical composition consisting of hydrogen, helium and traces of lithium1, almost all other elements were created in stars and supernovae. The mass fracti…

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