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University of Nevada, Las Vegas

Spectroscopic abundances of solar-type dwarfs in open cluster M34 (Ngc 1039)

Abstract

dc:description.abstract

Parameters and relative abundances of Fe, Ni, Ti, Cr, Ca, Si, Al, and Mg have been derived for nine M34 G and K dwarfs from high-resolution, modest S/N, Keck/HIRES spectra. Effective temperatures have been derived spectroscopically and fall in the range 4750 ≤ Teff ≤ 6130 K. Despite modest scatter in Fe, Ti, Cr, Ca, Al, and Mg (none of which is found to be correlated with Li scatter in M34), our two coolest stars are slightly though consistently underabundant in these elements relative to the warmer stars. The two cool stars are slightly overabundant in Si, whose abundances are derived from higher excitation lines. This and our finding that Fe II-based abundances are significantly higher than Fe I-based values in the cool stars seems to point towards the action of NLTE effects (overionization and/or overexcitation), though additional analysis is required to exclude inadequacies in the model atmospheres. Final mean cluster abundances are based on five warm stars, which indicate [Fe/H] = +0.07 +/- 0.04, and are void of any statistically significant scatter. The other elements scale well with Fe, except for Ni, which appears to be slightly underabundant with respect to Fe. K abundances are derived and show a surprising marked trend with temperature, which further supports our suspicion of the presence of NLTE effects. Moreover, the expected similar spectroscopic behavior of the neutral alkali resonance lines we employ suggests the apparent Li and K underabundances in cool M34 dwarfs are partly related; thus, some portion of the well-known Li-Teff trend in cool M34 dwarfs may be illusory.

Degree

thesis:*
Name thesis:degree_name
Master of Science (MS)
Level thesis:degree_level
Thesis
Discipline thesis:degree_discipline
Physics
Grantor dc:publisher
University of Nevada, Las Vegas
Year
2002

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Schuler, Simon Charles
Contributors dc:contributor
  • Jeremy R. King

Rights

dc:rights
Statement dc:rights
  • IN COPYRIGHT. For more information about this rights statement, please visit http://rightsstatements.org/vocab/InC/1.0/
Language dc:language
English

Identifiers

dc:identifier.*
OAI identifier oai:identifier
oai:oasis.library.unlv.edu:rtds-2442

Chain of custody

source
Harvested from
University of Nevada - Las Vegas
Base URL
oasis.library.unlv.edu/do/oai/
Last updated
2026-07-24
Source record
OAI-PMH GetRecord
related terms
citation

Schuler, Simon Charles. Spectroscopic abundances of solar-type dwarfs in open cluster M34 (Ngc 1039). Thesis thesis, University of Nevada, Las Vegas, 2002. https://doi.org/10.25669/henf-3ksq