Publication date
July 2023
DOIAbstract
Code and data to reproduce the results of AAS journals article "Left Ringing: Betelgeuse Illuminates the Connection Between Convective outbursts, Mode switching, and Mass Ejection in Red Supergiants
Code and data to reproduce the results of AAS journals article "Left Ringing: Betelgeuse Illuminates the Connection Between Convective outbursts, Mode switching, and Mass Ejection in Red Supergiants
Context. Despite being the best studied red supergiant star in our Galaxy, the physics behind the ph...
Aims. Understanding convection in red supergiants and the mechanisms that trigger the mass loss from...
The red supergiant star, Betelgeuse, was first reported to be dimming beyond its usual fluctuations ...
We conduct a rigorous examination of the nearby red supergiant Betelgeuse by drawing on the synthesi...
The nearby red supergiant (RSG) Betelgeuse has a complex circumstellar medium out to at least 0.5 pa...
Convection, pulsation and magnetic fields have all been suggested as mechanisms for the transport of...
© 2020. The American Astronomical Society. All rights reserved. Photometry available at https://konk...
The nearby red supergiant (RSG) Betelgeuse has a complex circumstellar medium out to at le...
The bright supergiant, Betelgeuse (Alpha Orionis, HD 39801), underwent a historic optical dimming du...
Red supergiants are the most common final evolutionary stage of stars that have initial masses betwe...
Betelgeuse is the brightest Red Supergiant (RSG) in the sky and thus has been studied over decades. ...
International audienceThe bright supergiant, Betelgeuse (Alpha Orionis, HD 39801), underwent a histo...
Understanding convection in red supergiants and the mechanisms that trigger the mass loss from these...
Context. Betelgeuse is an M supergiant with a complex and extended atmosphere, which also harbors sp...
The bright supergiant Betelgeuse (Alpha Orionis, HD 39801) experienced a visual dimming during 2019 ...
Context. Despite being the best studied red supergiant star in our Galaxy, the physics behind the ph...
Aims. Understanding convection in red supergiants and the mechanisms that trigger the mass loss from...
The red supergiant star, Betelgeuse, was first reported to be dimming beyond its usual fluctuations ...
We conduct a rigorous examination of the nearby red supergiant Betelgeuse by drawing on the synthesi...
The nearby red supergiant (RSG) Betelgeuse has a complex circumstellar medium out to at least 0.5 pa...
Convection, pulsation and magnetic fields have all been suggested as mechanisms for the transport of...
© 2020. The American Astronomical Society. All rights reserved. Photometry available at https://konk...
The nearby red supergiant (RSG) Betelgeuse has a complex circumstellar medium out to at le...
The bright supergiant, Betelgeuse (Alpha Orionis, HD 39801), underwent a historic optical dimming du...
Red supergiants are the most common final evolutionary stage of stars that have initial masses betwe...
Betelgeuse is the brightest Red Supergiant (RSG) in the sky and thus has been studied over decades. ...
International audienceThe bright supergiant, Betelgeuse (Alpha Orionis, HD 39801), underwent a histo...
Understanding convection in red supergiants and the mechanisms that trigger the mass loss from these...
Context. Betelgeuse is an M supergiant with a complex and extended atmosphere, which also harbors sp...
The bright supergiant Betelgeuse (Alpha Orionis, HD 39801) experienced a visual dimming during 2019 ...
Context. Despite being the best studied red supergiant star in our Galaxy, the physics behind the ph...
Aims. Understanding convection in red supergiants and the mechanisms that trigger the mass loss from...
The red supergiant star, Betelgeuse, was first reported to be dimming beyond its usual fluctuations ...
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