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Chromospheric activity and stellar evolution - Clues from IUE data
We investigate the dependence of chromospheric activity on stellarphysical parameters in a sample of cool giants and supergiants. Ca IIsurface fluxes for stars of known masses and evolutionary status arederived from published IUE Mg II observations. Adding these data to thesample of Pasquini et al. (1990) we find that chromospheric activity inevolved stars is better described by two stellar parameters, and a tightrelationship is found between activity, stellar Teff and Mass. Wediscuss this relationship arguing that the stellar evolutionary statuscould play a 'hidden' but fundamental role in determining the activitylevel of evolved late type stars.
| Determinations of the Parallaxes of Barnard's Star BD-70DEG68 and BD-4DEG4157
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Cassiopeia |
| Ascensió Recta: | 01h05m31.28s |
| Declinació: | +72°11'52.6" |
| Magnitud Aparent: | 9.209 |
| Moviment propi RA: | 16.1 |
| Moviment propi Dec: | -21.1 |
| B-T magnitude: | 9.756 |
| V-T magnitude: | 9.255 |
Catàlegs i designacions:
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