Radio evidence on the mass loss bi-stability jump

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dc.creatorBenaglia, P.
dc.creatorVink, J. S.
dc.creatorMarti, J.
dc.creatorMaiz-Apellaniz, J.
dc.creatorKoribalski, B.
dc.creatorJohnston, S.
dc.date2006-08-21
dc.date.accessioned2026-07-07T07:19:24Z
dc.date.available2026-07-07T07:19:24Z
dc.descriptionWe present the results of a first campaign of radio continuum observations toward supergiants with spectral types in the range O8 - B3. Three targets out of twelve were detected with the ATCA and the VLA. The measured fluxes and the upper limits yielded values of the stellar mass-loss rates dM/dt and the wind efficiencies. The comparison of predicted and derived values of dM/dt shows a good agreement.
dc.descriptionProceeding of the Conference Mass loss from stars and the evolution of stellar clusters
dc.identifierhttps://arxiv.org/abs/astro-ph/0608435
dc.identifierhttp://arxiv.org/abs/astro-ph/0608435
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/114611
dc.subjectAstrophysics
dc.titleRadio evidence on the mass loss bi-stability jump
dc.typetext

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