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researcher

S. Cristallo

127 papers hereh-index 395.6k citations317 works total

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

author position
  • sole author1
  • first author12
  • middle author85
  • last author14

Across the 112 of 127 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR79
  • nucl-ex16
  • astro-ph10
  • astro-ph.GA10
  • physics.ins-det6
  • astro-ph.HE3
same name
  • S. Cristallo — 6 papers
  • S. Cristallo — 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
20032026
most citedEvolution, nucleosynthesis and yields of low mass AGB stars

439 citations · 6.3k across the 124 of their papers we have counts for

collaborators
Showing 2008Show all

4 papers · 1 filter

astro-ph2008★ 62 cited

Fluorine in AGB Carbon Stars Revisited

C. Abia, A. Recio-Blanco, P. de Laverny +3

A reanalysis of the fluorine abundance in three Galactic AGB carbon stars (TX Psc, AQ Sgr and R Scl) has been performed from the molecular HF (1-0) R9 line at 2.3358 μm. High-res…

astro-ph2008

Evolution and nucleosynthesis in low mass Asymptotic Giant Branch stars

S. Cristallo

People usually smile when astrophysicists assert that we are sons of the stars, but human life confirms this sentence: about 65% of the mass of our body is made up of oxygen, carbo…

astro-ph2008★ 54 cited

AGB stars of the intermediate-age LMC cluster NGC 1846 II. Dredge up along the AGB

T. Lebzelter, M. T. Lederer, S. Cristallo +3

Aims: We investigate the change in the surface abundance of 12C during the evolution along the AGB, aiming to constrain third dredge-up models. Methods: High-resolution, near-…

astro-ph2008★ 40 cited

Fluorine in carbon-enhanced metal-poor stars: a binary scenario

M. Lugaro, S. E. de Mink, R. G. Izzard +8

A super-solar fluorine abundance was observed in the carbon-enhanced metal-poor (CEMP) star HE 1305+0132 ([F/Fe] = +2.90, [Fe/H] = -2.5). We propose that this observation can be ex…

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