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Context. Measurement of the Galactic neutral atomic hydrogen (H i) column density, N H i , and brightness temperatures, T B , is of high scientific value for a broad range of astrophysical disciplines. In the past two decades, one of the most-used legacy H i datasets has been the Leiden/Argentine/Bonn Survey (LAB).
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N. Ben Bekhti
University of Bonn
L. Flöer
University of Bonn
Reinhard Keller
Robert Bosch (Germany)
Astronomy and Astrophysics
University of Arizona
The University of Sydney
Australian National University
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Bekhti et al. (Sat,) studied this question.
synapsesocial.com/papers/69d81700a2a48916bbbeeedc — DOI: https://doi.org/10.1051/0004-6361/201629178
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