Parent Stars of Extrasolar Planets. XII. Additional evidence for trends with vsini, condensation temperature, and chromospheric activity

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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4 pages, 4 figures; accepted for publication in MNRAS as a Letter

Scientific paper

Several recent studies have reported differences in vsini,
abundance-condensation temperature trends, and chromospheric activity between
samples of stars with and without Doppler-detected planets. These findings have
been disputed, and the status of these results remains uncertain. We evaluate
these claims using additional published data and find support for all three.

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