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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