Cited by 41Galaxies: Formation, Evolution, PhenomenaStellar, planetary, and galactic studiesAstrophysics and Star Formation Studies

On variations in the fine-structure constant and stellar pollution of quasar absorption systems

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Fenner, Y., Murphy, M. T., Gibson, B. K.·2005·Monthly Notices of the Royal Astronomical Society

Abstract

At redshifts zabs≲ 2, quasar absorption-line constraints on space–time variations in the fine-structure constant, α, rely on the comparison of Mgii and Feii transition wavelengths. One potentially important uncertainty is the relative abundance of Mg isotopes in the absorbers, which, if different from solar, can cause spurious shifts in the measured wavelengths and, therefore, α. Here we explore chemical evolution models with enhanced populations of intermediate-mass (IM) stars, which, in their asymptotic giant branch phase, are thought to be the dominant factories for heavy Mg isotopes at the low metallicities typical of quasar absorption systems. By design, these models partially explain recent Keck/HIRES evidence for a smaller α in zabs < 2 absorption clouds than on Earth. However, such models also overproduce N, violating observed abundance trends in high-zabs damped Lyman-α (DLA) systems. Our results do not support the recent claim of Ashenfelter et al. that similar models of IM-enhanced initial mass functions (IMFs) may simultaneously explain the HIRES varying-α data and DLA N abundances. We explore the effect of the IM-enhanced model on Si, Al and P abundances, finding it to be much less pronounced than for N. We also show that the 13C/12C ratio, as measured in absorption systems, could constitute a future diagnostic of non-standard models of the high-redshift IMF.

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Crossref · 10.1111/j.1365-2966.2005.08781.x

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  • Such a modified nucleosynthetic history will lead to an overproduction of elements such as P, Si and Al above current constraints (Fenner et al. 2005).

    “However, such modified nucleosynthetic history will lead to an overproduction of elements such as P, Si, Al, P above current constraints (Fenner et al. 2005)”

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Research works printed but not linked: 2

  1. Levshakov S. A., Centurion M., Molaro P., D'Odorico S., 2004, A&amp;A, in press (astro-ph/0408188) · arXiv
  2. Milne E. A., 1937, Proc. R. Soc. A, 158, 324

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Authors
Fenner, Y., Murphy, M. T., & Gibson, B. K.
Affiliations
  • Swinburne University of Technology (AU)
  • University of Cambridge (GB)
Venue
Monthly Notices of the Royal Astronomical Society
Published
2005-04
Volume
358
Issue
2
Pages
468-480
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2009743323
Cited by
41
References
116
Citations by year
2025: 1 · 2024: 1 · 2022: 2 · 2021: 1 · 2020: 2 · 2019: 2 · 2018: 1 · 2017: 2 · 2016: 4 · 2014: 1 · 2013: 2 · 2012: 2
FWCI
2.71
Type
journal article
Language
en
Open access
Locations
  • Monthly Notices of the Royal Astronomical Society (publishedVersion)
  • Swinburne figshare (Swinburne University of Technology) (acceptedVersion)
  • Figshare (submittedVersion, cc-by)
  • Swinburne figshare (Swinburne University of Technology)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
Keywords
fine-structure constant variation, quasar absorption lines, stellar pollution, magnesium isotopes, intermediate-mass stars, chemical evolution models, damped Lyman-alpha systems, initial mass function, nitrogen abundance, carbon isotope ratio, asymptotic giant branch, high-redshift absorbers

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