Monitoring High Amplitude Delta Scuti Stars with a Small Telescope

Details Monitoring High Amplitude Delta Scuti Stars with a Small Telescope Monitoring High Amplitude Delta Scuti Stars with a Small Telescope

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.9003i&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #90.03; Bulletin of the American Astronomical Society, Vol. 33, p.1436

Astronomy and Astrophysics

Astronomy

Scientific paper

We're using a small aperture telescope and a relatively moderate time expenditure to obtain high quality CCD light curves of short-period variable stars. All data were obtained using 0.4 meter telescope, taking CCD observations in a standard V filter. Presented data are on 8 high amplitude delta Scuti stars (AD CMi, BS Aqr, CY Aqr, DY Her, DY Peg, EH Lib, XX Cyg, and YZ Boo) which are part of a larger ongoing project; monitoring a list of stars several times a year over the last decade, searching for variations in periods and/or pulsation amplitudes.

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