Résumé
We carried out an optical spectroscopic survey of twenty one stars to search for Ca II circumstellar gas at the stellar velocity similar to that found in the β Pictoris disk. The surveyed stars are A-type stars with large v sin i in the Ursa Major stellar kinematic group. No evidence of circumstellar gas was found around any of the stars. This result suggests that β Pictoris either is a very peculiar object surrounded by an anomalous amount of gas, or is younger than the stars in the Ursa Major Group (∼ 3 108 years).
| langue originale | Anglais |
|---|---|
| Pages (de - à) | 602-605 |
| Nombre de pages | 4 |
| journal | Astronomy and Astrophysics |
| Volume | 328 |
| Numéro de publication | 2 |
| état | Publié - 10 déc. 1997 |
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