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Title: Milky Way tomography with K and M dwarf stars: The vertical structure of the galactic disk

Journal Article · · The Astrophysical Journal (Online)
 [1];  [2];  [3]
  1. Univ. of Kentucky, Lexington, KY (United States)
  2. Univ. of Kentucky, Lexington, KY (United States); Univ. of California, Irvine, CA (United States)
  3. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

Here, we use the number density distributions of K and M dwarf stars with vertical height from the Galactic disk, determined using observations from the Sloan Digital Sky Survey (SDSS), to probe the structure of the Milky Way disk across the survey's footprint. Using photometric parallax as a distance estimator we analyze a sample of several million disk stars in matching footprints above and below the Galactic plane, and we determine the location and extent of vertical asymmetries in the number counts in a variety of thin and thick disk subsamples in regions of some 200 square degrees within 2 kpc in vertical distance from the Galactic disk. These disk asymmetries present wave-like features as previously observed on other scales and distances from the Sun. We additionally explore the scale height of the disk and the implied offset of the Sun from the Galactic plane at different locations, noting that the scale height of the disk can differ significantly when measured using stars only above or only below the plane. Moreover, we compare the shape of the number density distribution in the north for different latitude ranges with a fixed range in longitude and find the shape to be sensitive to the selected latitude window. We explain why this may be indicative of a change in stellar populations in the compared latitude regions, possibly allowing access to the systematic metallicity difference between thin and thick disk populations through photometry.

Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Organization:
DES
Grant/Contract Number:
AC02-07CH11359
OSTI ID:
1365572
Report Number(s):
FERMILAB-PUB-17-187-AE; 1607147
Journal Information:
The Astrophysical Journal (Online), Vol. 843, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 22 works
Citation information provided by
Web of Science

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The Milky Way Tomography with SDSS: II. Stellar Metallicity text January 2008
Hundreds of Milky Way Satellites? Luminosity Bias in the Satellite Luminosity Function text January 2008
The Invisibles: A Detection Algorithm to Trace the Faintest Milky Way Satellites text January 2008
SEGUE: A Spectroscopic Survey of 240,000 stars with g=14-20 text January 2009
The spiral structure of our Milky Way Galaxy text January 2009
The origin of large peculiar motions of star-forming regions and spiral structures of our Galaxy text January 2009
Dark matter substructure and dwarf galactic satellites text January 2009
Substructure depletion in the Milky Way halo by the disk text January 2009
Getting the astrophysics and particle physics of dark matter out of next-generation direct detection experiments text January 2009
Finding Dwarf Galaxies From Their Tidal Imprints text January 2011
Galactoseismology: Discovery of Vertical Waves in the Galactic Disk text January 2012
The wobbly Galaxy: kinematics north and south with RAVE red clump giants text January 2013
The Stellar Number Density Distribution in the Local Solar Neighborhood is North-South Asymmetric text January 2013
Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the Solar neighbourhood text January 2013
Substructure in bulk velocities of Milky Way disk stars text January 2013
Chemical Cartography with APOGEE: Large-scale Mean Metallicity Maps of the Milky Way text January 2013
The Besancon Galaxy model renewed I. Constraints on the local star formation history from Tycho data text January 2014
Bending and Breathing Modes of the Galactic Disk text January 2014
New Galactic embedded clusters and candidates from a WISE Survey text January 2014
The morphology of the Milky Way - I. Reconstructing CO maps from simulations in fixed potentials text January 2014
Constraining the thick disc formation scenario of the Milky Way text January 2014
Discovery of two embedded clusters with WISE in the high Galactic latitude cloud HRK 81.4-77.8 text January 2015
Planck 2015 results. XIII. Cosmological parameters text January 2015
A re-interpretation of the Triangulum-Andromeda stellar clouds: a population of halo stars kicked out of the Galactic disk text January 2015
Tracing the Galactic spiral structure with embedded clusters text January 2015
The vertical effects of disc non-axisymmetries from perturbation theory: the case of the Galactic bar text January 2015
A fully cosmological model of a Monoceros-like ring text January 2015
Modelling the Galactic disc: perturbed distribution functions in the presence of spiral arms text January 2016
New detections of embedded clusters in the Galactic halo text January 2016
The Ghost of Sagittarius and Lumps in the Halo of the Milky Way text January 2001
Origin of Radially Increasing Stellar Scaleheight in a Galactic Disk text January 2002
Evidence for coupling between the Sagittarius dwarf galaxy and the Milky Way warp text January 2003
The Spiral Structure of the Outer Milky Way in Hydrogen text January 2006
Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions text January 2006
An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data text January 2007
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Cited By (6)

A homogeneous sample of 34 000 M7−M9.5 dwarfs brighter than J = 17.5 with accurate spectral types journal March 2019
Testing gravity with wide binary stars like α Centauri journal July 2018
Origin of the Local Group satellite planes journal April 2018
How to Constrain Your M Dwarf. II. The Mass–Luminosity–Metallicity Relation from 0.075 to 0.70 Solar Masses journal January 2019
The Gaia –ESO Survey: Carbon Abundance in the Galactic Thin and Thick Disks journal January 2020
The Gaia-ESO Survey: Carbon Abundance in the Galactic Thin and Thick Disks text January 2020

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