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T. Morel

75 papers hereh-index 4221.6k citations223 works total

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

author position
  • sole author6
  • first author7
  • middle author36
  • last author3

Across the 52 of 75 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR40
  • astro-ph18
  • astro-ph.GA8
  • astro-ph.IM5
  • astro-ph.EP4
same name
  • T. Morel — 33 papers, h 10
  • T. Morel — 11 papers, h 7
  • T. Morel — 4 papers, h 6
  • T. Morel — 3 papers
  • T. Morel — 3 papers, h 4
  • T. Morel — 3 papers, h 6

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
19992023
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 12.9k across the 75 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.SRShow all

3 papers · 2 filters

astro-ph.SR2017★ 22 cited

Chemical abundances of fast-rotating massive stars. II. Interpretation and comparison with evolutionary models

Constantin Cazorla, Yaël Nazé, Thierry Morel +3

Aims: Past observations of fast-rotating massive stars exhibiting normal nitrogen abundances at their surface have raised questions about the rotational mixing paradigm. We revisit…

astro-ph.SR2017★ 29 cited

Weighing in on the masses of retired A stars with asteroseismology: K2 observations of the exoplanet-host star HD 212771

Tiago L. Campante, Dimitri Veras, Thomas S. H. North +12

Doppler-based planet surveys point to an increasing occurrence rate of giant planets with stellar mass. Such surveys rely on evolved stars for a sample of intermediate-mass stars (…

astro-ph.SR2017★ 28 cited

Chemical abundances of fast-rotating massive stars. I. Description of the methods and individual results

Constantin Cazorla, Thierry Morel, Yael Naze +4

Aims: Recent observations have challenged our understanding of rotational mixing in massive stars by revealing a population of fast-rotating objects with apparently normal surface…

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