β Pictoris: Planets and Pulsations

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The A5 dwarf star β Pictoris has been subject of numerous studies
because it addresses several questions of stellar astrophysics, like
stellar evolution, circumstellar disks, planet formation and pulsations.
With V = 3.86 mag, it falls within the observable magnitude range of
BRITE and is a promising target for this space mission.

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