Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.276..199k&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 276, Issue 1, pp. 199-205.
Astronomy and Astrophysics
Astronomy
19
Stars: Chemically Peculiar, Stars: Individual: Hd 40765, Stars: Oscillations, Delta Scuti
Scientific paper
We have discovered that HD 40765 is a singly periodic delta Scuti star pulsating in the fundamental or first overtone radial mode with a period of 4.070h. Its light variations are non-sinusoidal and have peak-to-peak amplitudes of DeltaB=0.21 mag and DeltaV=0.15 mag. This star is strongly metallic-lined. We classify the spectrum Fmp (kA7hF5mF5), where the `p' does not indicate peculiar in the Ap sense, but peculiar in the sense that the spectrum cannot be fully parametrized. HD 40765 is a large-amplitude delta Scuti star which is also a rho Puppis, or evolved Am, star. By comparison with rho Puppis itself, the inferred surface radial velocity variations are 14 km s^-1 peak-to-peak. This implies either (1) that such pulsation can be non-turbulent at the level of predicted diffusion velocities of order cm s^-1, or (2) that diffusion should be reconsidered as the sole explanation for the abundance anomalies in this star.
Garrison Robert F.
Hofmann G. F.
Koen Chris
Kurtz Don W.
Viranna N. B.
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