The HI Distribution Observed toward a Halo Region of the Milky Way

The HI Distribution Observed toward a Halo Region of the Milky Way

We use observations of the neutral atomic hydrogen (HI) 21-cm emission line to study the spatial distribution of the HI gas in a 80° × 90° region of the Galaxy halo. The HI column densities in the range of 3–11 × 10 20 cm − 2 have been estimated for some of the studied regio...

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Bibliographic Details
Main Authors:	Ericson López, Jairo Armijos, Mario Llerena, Franklin Aldás
Format:	Article
Language:	English
Published:	MDPI AG 2017-08-01
Series:	Galaxies
Subjects:	21-cm emission line Galaxy halo interstellar medium
Online Access:	https://www.mdpi.com/2075-4434/5/3/45

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