Stability of protoplanets around RU LUPI

Details Stability of protoplanets around RU LUPI Stability of protoplanets around RU LUPI

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..74..235e&link_type=abstract

Astrophysics and Space Science, vol. 74, no. 1, Jan. 1981, p. 235-241.

Astronomy and Astrophysics

Astrophysics

3

Cosmic Dust, Dynamic Stability, Gravitational Collapse, Orbit Perturbation, Protoplanets, T Tauri Stars, Condensation, Grains

Scientific paper

It is shown that the protoplanetary dust condensations around the T
Tauri star RU Lup, proposed by Gahm et al. (1974), would be unstable to
tidal disruption if they are bound only by gravitational forces. There
are extreme conditions under which the condensations would be stable,
but such conditions would easily be verifiable observationally.

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