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Cited by 135Stellar, planetary, and galactic studiesAstronomy and Astrophysical ResearchGalaxies: Formation, Evolution, Phenomena

The DOI matches its Crossref record.

Stellar mass and age determinations: I. Grids of stellar models from Z = 0.006 to 0.04 and M = 0.5 to 3.5 M ⊙ ⋆⋆⋆

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Mowlavi, N., Eggenberger, P., Meynet, G., Ekström, S., Georgy, C., Maeder, A., Charbonnel, C., Eyer, L.·2012·Astronomy & Astrophysics
DOI 10.1051/0004-6361/201117749
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Abstract

Aims. We present dense grids of stellar models suitable for comparison with observable quantities measured with great precision, such as those derived from binary systems or planet-hosting stars.

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Crossref · 10.1051/0004-6361/201117749

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  • More massive stars (M >~1.3 M⊙), such as F-type stars, rapidly evolve away from the main-sequence, a significant disadvantage for the evolution and sustainment of exolife.

    “More massive stars ( M ∼ > 1 . 3 M ⊙ ), such as F-type stars, are known to rapidly evolve away from the mainsequence (e.g., Meynet et al. 1993; Mowlavi et al. 2012), a significant disadvantage for the evolution and sustainment of exolife”

    From ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS (2016) · cites this paper as Mowlavi et al. 2012

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Cited by

Sorted by citations

  • ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS

    Cuntz, M., & Guinan, E. F. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/827/1/79 · Cited by 77

    “Ly-α serves as an excellent indicator for FUV emission because this emission line alone contributes 80–90% of the total stellar 3Based on studies by, e.g., Schröder & Smith (2008) and Mowlavi et al. (2012) it has been found that the effective temperature of the young Sun was ∼5600 K (G6–7 V).”
    BackgroundInfluential

Metadata

Authors
Mowlavi, N., Eggenberger, P., Meynet, G., Ekström, S., Georgy, C., Maeder, A., Charbonnel, C., & Eyer, L.
Affiliations
  • University of Geneva (CH)
  • École Normale Supérieure de Lyon (FR)
ORCID
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2012-04-26
Volume
541
Pages
A41
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
DOI
10.1051/0004-6361/201117749
OpenAlex
W4296393596
Cited by
135
References
0
Citations by year
2026: 9 · 2025: 2 · 2024: 5 · 2023: 6 · 2022: 6 · 2021: 6 · 2020: 6 · 2019: 8 · 2018: 14 · 2017: 8 · 2016: 25 · 2015: 9 · 2014: 12 · 2013: 14 · 2012: 5
FWCI
7.00
Type
journal article
Language
en
Open access
Locations
  • Astronomy and Astrophysics (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • Springer Link (Chiba Institute of Technology) (submittedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Keywords
stellar mass estimation, stellar age determination, stellar evolution models, binary stars, exoplanet host stars, stellar parameters

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Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

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