dc.creatorBenaglia, Paula
dc.creatorCappa, Cristina Elisabet
dc.creatorKoribalski, B. S.
dc.date2001-06-15
dc.date2021-09-01T15:03:40Z
dc.date.accessioned2023-07-15T02:51:26Z
dc.date.available2023-07-15T02:51:26Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/123953
dc.identifierissn:0004-6361
dc.identifierissn:1432-0746
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7463532
dc.descriptionA sample of OB stars (eleven Of, one O and one B supergiant) has been surveyed with the Australia Telescope Compact Array at 4.8 and 8.64 GHz with a resolution of ∼2"–4". Five stars were detected; three of them have negative spectral indices, consistent with non-thermal emission, and two have positive indices. The thermal radiation from HD 150135 and HD 163181 can be explained as coming from an optically thick ionized stellar wind. The non-thermal radiation from CD–47◦ 4551, HD 124314 and HD 150136 possibly comes from strong shocks in the wind itself and/or in the wind colliding region if the stars have a massive early-type companion. The percentage of non-thermal emitters among detected O stars has increased up to ∼50%. The Of star HD 124314 clearly shows flux density variations. Mass loss rates (or upper limits) were derived for all the observed stars and the results compared with non-radio measurements and theoretical predictions.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.descriptionInstituto Argentino de Radioastronomía
dc.formatapplication/pdf
dc.format952-962
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.subjectstars: early-type
dc.subjectstars: mass loss
dc.subjectstars: winds, outflows
dc.subjectradio continuum: stars
dc.titleMass loss rate determinations of southern OB stars
dc.typeArticulo
dc.typeArticulo


Este ítem pertenece a la siguiente institución