SIZING UP THE MILKY WAY: A BAYESIAN MIXTURE MODEL META-ANALYSIS OF PHOTOMETRIC SCALE LENGTH MEASUREMENTS

ABSTRACT The exponential scale length (Ld) of the Milky Way's (MW's) disk is a critical parameter for describing the global physical size of our Galaxy, important both for interpreting other Galactic measurements and helping us to understand how our Galaxy fits into extragalactic contexts....

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Bibliographic Details
Published in:The Astrophysical journal 2016-11, Vol.831 (1), p.71
Main Authors: Licquia, Timothy C., Newman, Jeffrey A.
Format: Article
Language:English
Subjects:
Astrophysics
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Bayesian analysis
COMPUTERIZED SIMULATION
DISTRIBUTION
Galactic disk
Galaxy: disk
Galaxy: fundamental parameters
Galaxy: structure
Infrared analysis
Infrared photometry
MASS
Meta-analysis
methods: statistical
MILKY WAY
PHOTOMETRY
Spiral galaxies
STATISTICS
Stellar mass
Systematic errors
Uncertainty analysis
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Summary:ABSTRACT The exponential scale length (Ld) of the Milky Way's (MW's) disk is a critical parameter for describing the global physical size of our Galaxy, important both for interpreting other Galactic measurements and helping us to understand how our Galaxy fits into extragalactic contexts. Unfortunately, current estimates span a wide range of values and are often statistically incompatible with one another. Here, we perform a Bayesian meta-analysis to determine an improved, aggregate estimate for Ld, utilizing a mixture-model approach to account for the possibility that any one measurement has not properly accounted for all statistical or systematic errors. Within this machinery, we explore a variety of ways of modeling the nature of problematic measurements, and then employ a Bayesian model averaging technique to derive net posterior distributions that incorporate any model-selection uncertainty. Our meta-analysis combines 29 different (15 visible and 14 infrared) photometric measurements of Ld available in the literature; these involve a broad assortment of observational data sets, MW models and assumptions, and methodologies, all tabulated herein. Analyzing the visible and infrared measurements separately yields estimates for Ld of kpc and kpc, respectively, whereas considering them all combined yields 2.64 0.13 kpc. The ratio between the visible and infrared scale lengths determined here is very similar to that measured in external spiral galaxies. We use these results to update the model of the Galactic disk from our previous work, constraining its stellar mass to be M , and the MW's total stellar mass to be M .
ISSN:0004-637X
1538-4357
DOI:10.3847/0004-637X/831/1/71