dc.creatorFariña, Cecilia
dc.creatorBosch, Guillermo Luis
dc.creatorMorrell, Nidia Irene
dc.creatorBarbá, Rodolfo Héctor
dc.creatorWalborn, Nolan Revere
dc.date2009
dc.date2019-10-04T17:09:51Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/82768
dc.identifierissn:0004-6256
dc.descriptionWe present a spectroscopic study of the N159/N160 massive star-forming region south of 30 Doradus in the Large Magellanic Cloud, classifying a total of 189 stars in the field of the complex. Most of them belong to O and early B spectral classes; we have also found some uncommon and very interesting spectra, including members of the Onfp class, a Be PCygni star, and some possible multiple systems. Using spectral types as broad indicators of evolutionary stages, we considered the evolutionary status of the region as a whole. We infer that massive stars at different evolutionary stages are present throughout the region, favoring the idea of a common time for the origin of recent star formation in the N159/N160 complex as a whole, while sequential star formation at different rates is probably present in several subregions.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.descriptionInstituto de Astrofísica de La Plata
dc.formatapplication/pdf
dc.format510-516
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectMagellanic Clouds
dc.subjectstars: early type
dc.subjectGalaxies: Starburst
dc.subjectH II regions
dc.subjectISM: individual: (N159/N160)
dc.titleSpectroscopic study of the N159/N160 complex in the Large Magellanic Cloud
dc.typeArticulo
dc.typeArticulo


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