Results 231 to 240 of about 1,192 (260)
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2014
This chapter presents a general view of stellar winds, the main observational evidences and driving mechanisms. An estimate is made of the mass loss rates for hot and cool stars. The chapter ends with some comments on the interaction of the winds with the interstellar medium and the effects of winds on the evolution of the stars.
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This chapter presents a general view of stellar winds, the main observational evidences and driving mechanisms. An estimate is made of the mass loss rates for hot and cool stars. The chapter ends with some comments on the interaction of the winds with the interstellar medium and the effects of winds on the evolution of the stars.
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Destination exoplanet: Habitability conditions influenced by stellar winds properties
Astronomische Nachrichten, 2022J D Alvarado-Gomez +2 more
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2018
The tidally influenced secondary stars in interacting binaries are rapidly rotating and possess convective envelopes or are fully convective. This makes the generation of large-scale magnetic fields in such stars very likely, and magnetically influenced wind flows from the stellar surface would then lead to magnetic braking. The secondary would be spun
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The tidally influenced secondary stars in interacting binaries are rapidly rotating and possess convective envelopes or are fully convective. This makes the generation of large-scale magnetic fields in such stars very likely, and magnetically influenced wind flows from the stellar surface would then lead to magnetic braking. The secondary would be spun
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Alfvén waves as a driving mechanism in stellar winds
Advances in Space Research, 2010Vera Jatenco-Pereira
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The interaction of the solar wind and stellar winds with the partially ionized interstellar medium
Physics of Plasmas, 2001Wood B E, Zank G P
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Galactic Centre stellar winds and Sgr A* accretion
Monthly Notices of the Royal Astronomical Society, 2006Volker Springel +2 more
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