High-energy emission and its variability in young stellar objects
Argiroffi, C., High-energy emission and its variability in young stellar objects, Astronomische Nachrichten, 340, 284-289 (2019) (ADS)
(click on the image for a larger version)
How a young stellar object might drive an accretion flow into the star,
producing a flare.
An unrestricted free-fall stream might arrive with 300-500 km/s velocity,
resulting in a termination shock.
Would this be analogous to our solar
thick-target model,
perhaps?
Or, it may more nearly resemble a
Hyder flare.
How a young stellar object might drive an accretion flow into the star, producing a flare. An unrestricted free-fall stream might arrive with 300-500 km/s velocity, resulting in a termination shock. Would this be analogous to our solar thick-target model, perhaps? Or, it may more nearly resemble a Hyder flare.