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Physical parameters and pulsational mode of short-period small-amplitude Cepheids
Nine galactic short-period (P less than 8 days) small-amplitude Cepheidshave been the subject of a study to determine their physical parametersand pulsational properties. UBVRI photometry and radial velocities wereobtained in the same observing seasons. The wings of H-alpha were usedto determine effective temperatures. Empirical radii, luminosities, andmasses were determined. The short-period stars lie inside and seem to beon the red side of the observational Cepheid instability strip. It wasfound that these stars are likely pulsating in the radial fundamentalmode except HR 8084 (DT Cyg) which is suspected to be a first overtonepulsator. As the small-amplitude Cepheids in the LMC are thought to befirst overtone pulsators, it is suggested that small-amplitudesinusoidal variations are not the consequence of pulsation in the firstovertone, but rather the response to a more general amplitude trendacross the instability strip in a particular galactic system.
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Observation and Astrometry data
| Constellation: | Aquila |
| Right ascension: | 19h12m37.48s |
| Declination: | +05°17'50.5" |
| Apparent magnitude: | 7.737 |
| Proper motion RA: | -3.6 |
| Proper motion Dec: | 41.7 |
| B-T magnitude: | 8.989 |
| V-T magnitude: | 7.841 |
Catalogs and designations:
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