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South galactic CAP G and K stars with infrared excesses
Near-infrared and IRAS photometry is discussed for 13 G and K stars inthe south galactic cap. Five of them show a strong flux excess at 12microns as would be expected from dust shells emitting at temperaturesof several hundred Kelvin. One of them (XY Tau) has previously beenclassified as a 206-d Mira, but the new observations suggest it isactually a variable F or G star. The most likely explanation is that theoriginal classification was wrong and that it is in fact apremain-sequence star. The other four stars are either in very unusualevolutionary states or they are binary systems. The presence oflong-term variations in the near-infrared flux of the flare star CC Eriis reported. The colors are redder when the star is fainter, and thevariations might be associated with the star spot cycle.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Pegasus |
| Ascensió Recta: | 23h40m42.94s |
| Declinació: | +25°47'18.1" |
| Magnitud Aparent: | 8.316 |
| Distancia: | 534.759 parsecs |
| Moviment propi RA: | 5 |
| Moviment propi Dec: | -11.8 |
| B-T magnitude: | 10.498 |
| V-T magnitude: | 8.497 |
Catàlegs i designacions:
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