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HD 35606


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The Pulsation of EE Camelopardalis
EE Cam is a previously little-studied δ Scuti pulsator withamplitudes between those of the HADS (high-amplitude δ Scuti star)group and average low-amplitude pulsators. Since the size of stellarrotation determines both which pulsation modes are selected by the staras well as their amplitudes, this star offers a great opportunity toexamine the astrophysical connections. Extensive photometricmeasurements covering several months were carried out. Fifteensignificant pulsation frequencies were extracted. The dominant mode at4.934 cycles day-1 was identified as a radial mode byexamining the phase shifts at different wavelengths. Medium-dispersionspectra yielded a v sin i value of 40 ± 3 km s-1. Thisshows that EE Cam belongs to the important transition region betweenHADSs and normal δ Scuti stars.

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Observation and Astrometry data

Constellation:Καμηλοπάρδαλις
Right ascension:05h30m35.52s
Declination:+63°57'17.9"
Apparent magnitude:8.143
Distance:102.249 parsecs
Proper motion RA:-19.8
Proper motion Dec:5.8
B-T magnitude:8.763
V-T magnitude:8.195

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 35606
TYCHO-2 2000TYC 4089-903-1
USNO-A2.0USNO-A2 1500-04241293
HIPHIP 25800

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