Abstract
From the analysis of sensitive HI 21-cm line observations, we find evidence for vertically extended HI emission (|z|
Cite
CITATION STYLE
APA
Matthews, L. D., & Wood, K. (2003). High‐Latitude H i in the Low Surface Brightness Galaxy UGC 7321. The Astrophysical Journal, 593(2), 721–732. https://doi.org/10.1086/376602
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