Eight new δ Scuti stars

Details Eight new δ Scuti stars Eight new δ Scuti stars

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999mnras.309.1051k&link_type=abstract

Monthly Notices, Volume 309, Issue 4, pp. 1051-1062.

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Scientific paper

HD 23194, a member of the Pleiades, was found to pulsate with a period of about 30min. The literature on the star is reviewed, and it is concluded that it may be a marginal Am star in a binary system. HD 95321 is an evolved Am (ρ Puppis) star with a 5.1-h periodicity. Mode identification of its pulsation, based on multicolour photometry, suggests that the oscillation is probably non-radial with l=2. We also report on the discovery of six other new δ Scuti stars, some of which may be pulsating in gravity modes.

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