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dc.date.accessioned 2019-06-11T22:54:29Z
dc.date.available 2019-06-11T22:54:29Z
dc.date.issued 2008
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/76271
dc.description.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
dc.language en es
dc.subject Galaxias es
dc.title UBV-IR photometry and optical spectroscopy of the galactic OB association Bochum 7 en
dc.type Articulo es
sedici.identifier.uri http://www.astroscu.unam.mx/rmaa/RMxAC..33/PDF/RMxAC..33_mcorti.pdf es
sedici.identifier.other http://hdl.handle.net/11746/4474
sedici.creator.person Corti, Mariela Alejandra es
sedici.creator.person Bosch, Guillermo es
sedici.creator.person Niemelä, Virpi Sinikka es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-nd/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) es
sedici.relation.journalVolumeAndIssue vol. 33 es


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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)