How axi-symmetric is the inner HI disc of the Milky Way?
We modelled the distribution and the kinematics of HI in the inner Milky Way (R < R☉) at latitude b = 0∘ assuming axi-symmetry. We fitted the line profiles of the LAB 21-cm survey using an iterative approach based on the tangent-point method. The resulting model reproduces the H I data remarkabl...
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2012-02-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20121908007 |
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doaj-b94939aea78444a992199f53e9bdf3b52021-08-02T04:07:39ZengEDP SciencesEPJ Web of Conferences2100-014X2012-02-01190800710.1051/epjconf/20121908007How axi-symmetric is the inner HI disc of the Milky Way?Marasco A.Fraternali F.We modelled the distribution and the kinematics of HI in the inner Milky Way (R < R☉) at latitude b = 0∘ assuming axi-symmetry. We fitted the line profiles of the LAB 21-cm survey using an iterative approach based on the tangent-point method. The resulting model reproduces the H I data remarkably well, with significant differences arising only for R ≲ 2 kpc. This suggests that, despite the presence of a barred potential, the neutral gas in the inner Milky Way is distributed in a fairly axi-symmetric disc. http://dx.doi.org/10.1051/epjconf/20121908007 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Marasco A. Fraternali F. |
spellingShingle |
Marasco A. Fraternali F. How axi-symmetric is the inner HI disc of the Milky Way? EPJ Web of Conferences |
author_facet |
Marasco A. Fraternali F. |
author_sort |
Marasco A. |
title |
How axi-symmetric is the inner HI disc of the Milky Way? |
title_short |
How axi-symmetric is the inner HI disc of the Milky Way? |
title_full |
How axi-symmetric is the inner HI disc of the Milky Way? |
title_fullStr |
How axi-symmetric is the inner HI disc of the Milky Way? |
title_full_unstemmed |
How axi-symmetric is the inner HI disc of the Milky Way? |
title_sort |
how axi-symmetric is the inner hi disc of the milky way? |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2012-02-01 |
description |
We modelled the distribution and the kinematics of HI in the inner Milky Way (R < R☉) at latitude b = 0∘ assuming axi-symmetry. We fitted the line profiles of the LAB 21-cm survey using an iterative approach based on the tangent-point method. The resulting model reproduces the H I data remarkably well, with significant differences arising only for R ≲ 2 kpc. This suggests that, despite the presence of a barred potential, the neutral gas in the inner Milky Way is distributed in a fairly axi-symmetric disc. |
url |
http://dx.doi.org/10.1051/epjconf/20121908007 |
work_keys_str_mv |
AT marascoa howaxisymmetricistheinnerhidiscofthemilkyway AT fraternalif howaxisymmetricistheinnerhidiscofthemilkyway |
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