It is sometimes surmised that star-disc encounters may be a sufficient - or even necessary - condition for self-gravitating discs to fragment and form planets via gravitational instability. Our recent simulations support neither of these hypotheses. We find that discs whose thermal timescale is sufficiently long that they do not fragment in isolation are also stable against fragmentation during an encounter. We moreover find that if the disc enters a regime of relatively short cooling timescale, fragmentation does not require that this regime is entered rapidly. Consequently, discs will fragment if they enter the regime of rapid cooling by secular evolution, and impulsive changes - such as those resulting from an encounter - are not necessary. We thus conclude that planet formation is not promoted by a cluster environment.

Star-disc encounters and their role in planet formation / C.J. Clarke, E. Harper Clark, F. Meru, G. Lodato - In: Extreme solar systems / [a cura di] D. Fischer, F. A. Rasio, S. E. Thorsett, A. Wolszczan. - [s.l] : Astronomical Society of the Pacific, 2008. - ISBN 978-1-58381-666-0. - pp. 341 (( convegno Extreme solar systems tenutosi a Santorini, Grecia nel 2007.

Star-disc encounters and their role in planet formation

G. Lodato
Ultimo
2008

Abstract

It is sometimes surmised that star-disc encounters may be a sufficient - or even necessary - condition for self-gravitating discs to fragment and form planets via gravitational instability. Our recent simulations support neither of these hypotheses. We find that discs whose thermal timescale is sufficiently long that they do not fragment in isolation are also stable against fragmentation during an encounter. We moreover find that if the disc enters a regime of relatively short cooling timescale, fragmentation does not require that this regime is entered rapidly. Consequently, discs will fragment if they enter the regime of rapid cooling by secular evolution, and impulsive changes - such as those resulting from an encounter - are not necessary. We thus conclude that planet formation is not promoted by a cluster environment.
2008
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/58496
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