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Outflowing disk formation in B supergiants due to rotation and bi-stability in radiation driven winds

Curé, M.; Rial, D. F.; Cidale, Lydia Sonia (2005)

Massive stellar models: rotational evolution, metallicity effects

Ekström, Sylvia; Georgy, Cyril; Meynet, Georges; Maeder, André; Granada, Anahí (2011)

Slow radiation-driven wind solutions of A-type supergiants

Curé, M.; Cidale, Lydia Sonia; Granada, Anahí (2011)

The Slow Winds of A-Type Supergiants

Granada, Anahí; Curé, Michel; Cidale, Lydia Sonia (2010)

Chasing discs around O-type (proto)stars: ALMA evidence for an SiO disc and disc wind from G17.64+0.16

Maud L.T.; Cesaroni R.; Kumar M.S.N.; Van Der Tak F.F.S.; Allen V.; Hoare M.G.; Klaassen P.D.; Harsono D.; Hogerheijde M.R.; Sánchez-Monge A.; Schilke P.; Ahmadi A.; Beltrán M.T.; Beuther H.; Csengeri T.; Etoka S.; Fuller G.; Galván-Madrid R.; Goddi C.; Henning T.; Johnston K.G.; Kuiper R.; Lumsden S.; Moscadelli L.; Mottram J.C.; Peters T.; Rivilla V.M.; Testi L.; Vig S.; De Wit W.J.; Zinnecker H. (EDP Sciences, 2018)

Outflowing disk formation in B[e] supergiants due to rotation and bi-stability in radiation driven winds

Cure, M.; Rial, D.; Cidale, Lydia Sonia (EDP Sciences, 2005-07)

The effects of rapid rotation and bi-stability upon the density contrast between the equatorial and polar directions of a B[e] supergiant are re-investigated. Based on a new slow solution for different high rotational ...

Analytical solutions for radiation-driven winds in massive stars: I. the fast regime

Araya, I.; Curé, M.; Cidale, Lydia Sonia (Iop Publishing, 2014-10)

Accurate mass-loss rate estimates are crucial keys in the study of wind properties of massive stars and for testing different evolutionary scenarios. From a theoretical point of view, this implies solving a complex set of ...

Equatorial outflows driven by jets in Population III microquasars

Sotomayor Checa, Pablo Omar; Romero, Gustavo Esteban; Bosch-Ramon, Valentí (2021)

Limb-darkened radiation-driven winds from massive stars

Curé, Michel; Cidale, Lydia Sonia; Rial, D. F. (2012)

Modelling the line variations from the wind-wind shock emissions of WR 30a

FALCETA-GONCALVES, D.; ABRAHAM, Z.; JATENCO-PEREIRA, V. (BLACKWELL PUBLISHING, 2008)

The study of Wolf-Rayet stars plays an important role in evolutionary theories of massive stars. Among these objects, similar to 20 per cent are known to be in binary systems and can therefore be used for the mass determination ...

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