C.D.S. - SIMBAD4 rel 1.7 - 2021.02.26CET06:17:20

2008A&A...487..951K - Astronomy and Astrophysics, volume 487, 951-963 (2008/9-1)

Global properties of the HI distribution in the outer Milky Way. Planar and extra-planar gas.


Abstract (from CDS):

The determination of the global structure of the planar and extra-planar Milky Way H i disk depends critically on a reliable database but also on reasonable assumptions about the shape of the Milky Way rotation curve. We derive the 3D H i volume density distribution for the Galactic disk out to R ∼60 kpc. Our analysis is based on parameters for the warp and rotation curve derived previously. The data are taken from the Leiden/Argentine/Bonn all sky 21 cm line survey. The Milky Way H i disk is significantly warped but shows a coherent structure out to R ∼35 kpc. The radial surface density distribution, the densities in the middle of the warped plane, and the H i scale heights all follow exponential relations. The radial scale length for the surface density distribution of the H i disk is 3.75 kpc. Gas at the outskirts for 40 ≲R ≲60 kpc is described best by a distribution with an exponential radial scale length of 7.5 kpc and a velocity dispersion of 74 km/s. Such a highly turbulent medium fits also well with the average shape of the high velocity profile wings observed at high latitudes. The turbulent pressure gradient of such extra-planar gas is on average in balance with the gravitational forces. About 10% of the Milky Way H i gas is in this state. The large scale H i distribution is lopsided; for R > 15 kpc there is more gas in the south. The H i flaring indicates that this asymmetry is caused by a dark matter wake, located at R ∼25 kpc in direction of the Magellanic System. The H i disk is made up of two major components. Most prominent is the normal H i disk which can be traced to R ∼35 kpc. This is surrounded by a patchy distribution of highly turbulent gas reaching large scale heights but also large radial distances. At the position of the Sun the exponential scale height in the z direction is 3.9 kpc. This component resembles the anomalous gas discovered previously in some galaxies.

Abstract Copyright:

Journal keyword(s): Galaxy: disk - Galaxy: halo - Galaxy: structure - Galaxy: kinematics and dynamics - ISM: structure

Simbad objects: 5

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Number of rows : 5

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
1 NAME Magellanic Stream HVC 00 32 -30.0           ~ 838 1
2 NGC 891 H2G 02 22 32.907 +42 20 53.95 11.08 10.81 9.93 7.86   ~ 1548 2
3 NGC 2403 AGN 07 36 51.396 +65 36 09.17 9.31 8.84 8.38 8.19   ~ 1637 1
4 NGC 3198 EmG 10 19 54.990 +45 32 58.88 10.83 10.87 10.33     ~ 830 1
5 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11994 0

    Equat.    Gal    SGal    Ecl

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