UBV-IR photometry and optical spectroscopy of the galactic OB association Bochum 7

cic.isFulltext true es
cic.isPeerReviewed true es
cic.lugarDesarrollo Facultad de Ciencias Astronómicas y Geofísicas es
cic.version info:eu-repo/semantics/publishedVersion es
dc.date.accessioned 2016-10-21T17:03:54Z
dc.date.available 2016-10-21T17:03:54Z
dc.identifier.uri https://digital.cic.gba.gob.ar/handle/11746/4474
dc.title UBV-IR photometry and optical spectroscopy of the galactic OB association Bochum 7 en
dc.type Artículo es
dcterms.abstract The lack of tightly bound and easily identifiable young open clusters leads to the quest for OB associations as tracers of spiral arms. Massive stars are usually found in groups, and the presence of a WolfRayet star, WR12 in the catalogue of galactic WR stars (van der Hucht 2001), at α=8h44m47.2s , δ=−45◦58’55.5” (J2000.0), triggered the search for an surrounding OB association, now known as Bochum7 (Moffat & Vogt 1975). en
dcterms.creator.author Corti, Mariela es
dcterms.creator.author Bosch; G. L. es
dcterms.creator.author Niemela, Virpi S. es
dcterms.extent p. 52-52 es
dcterms.identifier.url Documento completo es
dcterms.isPartOf.issue vol. 33 es
dcterms.isPartOf.series Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) es
dcterms.issued 2008
dcterms.language Inglés es
dcterms.license Attribution-NonCommercial-NoDerivatives 4.0 International (BY-NC-ND 4.0) es
dcterms.publisher Instituto de Astronomía (UNAM) es
dcterms.subject.materia Astronomía es
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