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P. Molaro

22 papers hereh-index 6841 citations17 works total

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

author position
  • first author1
  • middle author15
  • last author3

Across the 19 of 22 papers where every author was matched, so the position is known.

fields
  • astro-ph7
  • astro-ph.SR7
  • astro-ph.GA6
  • astro-ph.EP1
  • astro-ph.HE1
same name
  • P. Molaro — 191 papers, h 51
  • 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
19992026
most citedMeasurement of stellar age from uranium decay

381 citations · 1.7k across the 22 of their papers we have counts for

collaborators
Showing 2011Show all

3 papers · 1 filter

astro-ph.SR2011★ 18 cited

Extremely metal-poor stars in SDSS fields

Piercarlo Bonifacio, Elisabetta Caffau, Patrick François +12

Some insight on the first generation of stars can be obtained from the chemical composition of their direct descendants, extremely metal-poor stars (EMP), with metallicity less tha…

astro-ph.SR2011★ 53 cited

First stars XIII. Two extremely metal-poor RR Lyrae stars?

C. J. Hansen, B. Nordstroem, P. Bonifacio +11

The chemical composition of extremely metal-poor stars (EMP stars; [Fe/H]<~ -3) is a unique tracer of early nucleosynthesis in the Galaxy. As such stars are rare, we wish to find c…

astro-ph.SR2011★ 50 cited

First Stars XIV. Sulfur abundances in extremely metal-poor (EMP) stars

Monique Spite, E. Caffau, S. M. Andrievsky +15

Sulfur is important: the site of its formation is uncertain, and at very low metallicity the trend of [S/Fe] against [Fe/H] is controversial. Below [Fe/H]=-2.0, [S/Fe] remains cons…

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