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The MAIA candidate star HD 208727
HD 208727 is a suspected member of the enigmatic MAIA variables andshows the largest yet observed amplitude in light variation for any ofthe potential members. Proven beyond doubt pulsation would pose aserious problem for stellar modelling and opacities, because eitheropacity source for driving pulsation has to be a different or newidentified, yet unkown, pulsation mechanism. We conclude from ourinvestigation that rotation is a more likely explanation for the lightvariability of HD 208727.
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Member of following groups:
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Observation and Astrometry data
| Constellation: | Paon |
| Right ascension: | 18h59m58.48s |
| Declination: | -71°55'57.5" |
| Apparent magnitude: | 6.784 |
| Distance: | 192.308 parsecs |
| Proper motion RA: | 19.3 |
| Proper motion Dec: | -22.5 |
| B-T magnitude: | 6.742 |
| V-T magnitude: | 6.781 |
Catalogs and designations:
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