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Kinematic and spatial distributions of barium stars - Are the barium stars and AM stars related?
The possibility of an evolutionary link between Am stars and bariumstars is considered, and an examination of previous data suggests thatbarium star precursors are main-sequence stars of intermediate mass, aremost likely A and/or F dwarfs, and are intermediate-mass binaries withclose to intermediate orbital separations. The possible role of masstransfer in the later development of Am systems is explored. Masstransfer and loss from systems with a range of masses and orbitalseparations may explain such statistical peculiarities of barium starsas the large dispersion in absolute magnitude, the large range ofelemental abundances from star to star, and the small number of starswith large peculiar velocities.
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Osservazione e dati astrometrici
| Costellazione: | Eridano |
| Ascensione retta: | 03h28m29.44s |
| Declinazione: | -41°12'18.3" |
| Magnitudine apparente: | 9.284 |
| Moto proprio RA: | 31.4 |
| Moto proprio Dec: | 153.7 |
| B-T magnitude: | 9.909 |
| V-T magnitude: | 9.336 |
Cataloghi e designazioni:
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