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

Detalhes bibliográficos
Autor(a) principal: Vieira, Edemundo da Rocha
Data de Publicação: 1971
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/109040
Resumo: 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.
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spelling Vieira, Edemundo da Rocha2015-01-20T02:15:08Z19710067-0049http://hdl.handle.net/10183/109040000122542We 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.application/pdfengThe Astrophysical journal. Supplement series. Chicago. Vol. 22, (Feb. 1971), p. 369-388Astrofisica do meio interestelarMateria interestelarRadioastronomiaMaps of the distribution of atomic hydrogen in a region in centaurusEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL000122542.pdf000122542.pdfTexto completo (inglês)application/pdf739199http://www.lume.ufrgs.br/bitstream/10183/109040/1/000122542.pdf5436e04c935db38929231c8131af7e81MD51TEXT000122542.pdf.txt000122542.pdf.txtExtracted Texttext/plain418http://www.lume.ufrgs.br/bitstream/10183/109040/2/000122542.pdf.txt5c7d268bf4dd690a39cdc92ac676ff51MD52THUMBNAIL000122542.pdf.jpg000122542.pdf.jpgGenerated Thumbnailimage/jpeg1883http://www.lume.ufrgs.br/bitstream/10183/109040/3/000122542.pdf.jpg92e2082421b54012952e3b0a9897cc37MD5310183/1090402018-10-23 08:41:53.001oai:www.lume.ufrgs.br:10183/109040Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2018-10-23T11:41:53Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Maps of the distribution of atomic hydrogen in a region in centaurus
title Maps of the distribution of atomic hydrogen in a region in centaurus
spellingShingle Maps of the distribution of atomic hydrogen in a region in centaurus
Vieira, Edemundo da Rocha
Astrofisica do meio interestelar
Materia interestelar
Radioastronomia
title_short Maps of the distribution of atomic hydrogen in a region in centaurus
title_full Maps of the distribution of atomic hydrogen in a region in centaurus
title_fullStr Maps of the distribution of atomic hydrogen in a region in centaurus
title_full_unstemmed Maps of the distribution of atomic hydrogen in a region in centaurus
title_sort Maps of the distribution of atomic hydrogen in a region in centaurus
author Vieira, Edemundo da Rocha
author_facet Vieira, Edemundo da Rocha
author_role author
dc.contributor.author.fl_str_mv Vieira, Edemundo da Rocha
dc.subject.por.fl_str_mv Astrofisica do meio interestelar
Materia interestelar
Radioastronomia
topic Astrofisica do meio interestelar
Materia interestelar
Radioastronomia
description 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.
publishDate 1971
dc.date.issued.fl_str_mv 1971
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dc.relation.ispartof.pt_BR.fl_str_mv The Astrophysical journal. Supplement series. Chicago. Vol. 22, (Feb. 1971), p. 369-388
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