Maps of the distribution of atomic hydrogen in a region in centaurus

dc.contributor.author	Vieira, Edemundo da Rocha	pt_BR
dc.date.accessioned	2015-01-20T02:15:08Z	pt_BR
dc.date.issued	1971	pt_BR
dc.identifier.issn	0067-0049	pt_BR
dc.identifier.uri	http://hdl.handle.net/10183/109040	pt_BR
dc.description.abstract	We have made a survey of the region 302° ≤ l ≤ 310°, 2° ≤ b ≤ 12° at the frequency of the hydrogen line. We have detected three elongated features that run parallel to the galactic plane at heights of about 200 pc above it, two of which may be associated with spiral arms in the plane. In addition, we have observed a number of very small clouds with negative radial velocities and one cloud with positive radial velocity.	en
dc.format.mimetype	application/pdf
dc.language.iso	eng	pt_BR
dc.relation.ispartof	The Astrophysical journal. Supplement series. Chicago. Vol. 22, (Feb. 1971), p. 369-388	pt_BR
dc.rights	Open Access	en
dc.subject	Astrofisica do meio interestelar	pt_BR
dc.subject	Materia interestelar	pt_BR
dc.subject	Radioastronomia	pt_BR
dc.title	Maps of the distribution of atomic hydrogen in a region in centaurus	pt_BR
dc.type	Artigo de periódico	pt_BR
dc.identifier.nrb	000122542	pt_BR
dc.type.origin	Estrangeiro	pt_BR

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