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A bayesian approach to the vertical structure of the disk of the Milky Way

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Title: A bayesian approach to the vertical structure of the disk of the Milky Way
Authors: Dobbie, PS
Warren, SJ
Item Type: Journal Article
Abstract: This work investigates the vertical profile of the stars in the disk of the Milky Way. The models investigated are of the form sech2/n(nz/(2H)) where, setting α = 2/n, the three functions of the sequence α= 0, 1, 2 correspond to exponential, sech, and sech2 functions respectively. We consider symmetric models and asymmetric models, above and below the plane. The study uses the large sample of K and M stars of Ferguson et al. (2017) and applies the methods of Bayesian model comparison to discriminate between the 6 models. Two inconsistencies in Ferguson et al. (2017), concerning the vertical height cut and the model continuity across the plane, are noted and addressed. We find that (1) in the Milky Way the symmetric disc models are decisively ruled out, with northern thin disc scale heights about 25% larger than southern, (2) there is moderate evidence for the exponential and sech models over the sech2 model, though a sample extending further into the Galactic mid-plane is needed to strengthen this result, (3) the photometric distances used by Ferguson et al. underestimate the GAIA distances by a factor of roughly 1.16, and (4) the increase of scale height with Galactic latitude observed by Ferguson et al. is due to incorrect cuts to the data.
Issue Date: 23-Jun-2020
Date of Acceptance: 23-Jun-2020
URI: http://hdl.handle.net/10044/1/80490
DOI: 10.21105/astro.2003.05757
ISSN: 2565-6120
Publisher: The Open Journal
Journal / Book Title: The Open Journal of Astrophysics
Volume: 3
Issue: 1
Copyright Statement: © 2020 The Author(s). This is an open-access article distributed under the terms of the Creative Commons Attribution 4.0 International License (CCBY-4.0) (http://creativecommons.org/licenses/by/4.0). View this license’s legal deed and legal code for more information
Keywords: astro-ph.GA
astro-ph.GA
Publication Status: Published
Online Publication Date: 2020-06-23
Appears in Collections:Physics
Astrophysics