Studying the Variation of the Fine Structure Constant Using Emission Line Multiplets

Abstract

As an extension of the method by Bahcall et al. (2004) to investigate the time dependence of the fine structure constant, we describe an approach based on new observations of forbidden line multiplets from different ionic species. We obtain optical spectra of fine structure transitions in [Ne III], [Ne V], [O III], [OI], and [SII] multiplets from a sample of 14 Seyfert 1.5 galaxies in the low-z range 0.035 < z < 0.281. Each source and each multiplet is independently analyzed to ascertain possible errors. Averaging over our sample, we obtain a conservative value alpha^2(t)/α^2(0) = 1.0030+-0.0014. However, our sample is limited in size and our fitting technique simplistic as we primarily intend to illustrate the scope and strengths of emission line studies of the time variation of the fine structure constant. The approach can be further extended and generalized to a "many-multiplet emission line method" analogous in principle to the corresponding method using absorption lines. With that aim, we note that the theoretical limits on emission line ratios of selected ions are precisely known, and provide well constrained selection criteria. We also discuss several other forbidden and allowed lines that may constitute the basis for a more rigorous study using high-resolution instruments on the next generation of 8 m class telescopes.

20 pages, 4 figures, sumbitted to AJ

References in corpus (7)

• New limit on the present temporal variation of the fine structure constant
• Early Growth and Efficient Accretion of Massive Black Holes at High Redshift
• A Complete Sample of Soft X-ray Selected AGN: II. Statistical Analysis
• A Complete Sample of Soft X-ray Selected AGN: I. The Data
• A Reexamination of Electron Density Diagnostics for Ionized Gaseous Nebulae
• Implications of Quasar Black Hole Masses at High Redshifts
• Theoretical FeI/II/III Emission-Line Strengths from Active Galactic Nuclei with Broad-Line Regions

Cited by in corpus (7)

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• Time variation of the fine structure constant in the early universe and the Bekenstein model
• The value of the fine structure constant over cosmological times
• Line and Continuum Variability in Active Galaxies
• Nonlinear electrodynamics and the variation of the fine structure constant
• The time variation of the fine structure constant: A statistical analysis of astronomical data