Abstract
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).
| Original language | English |
|---|---|
| Pages (from-to) | 602-605 |
| Number of pages | 4 |
| Journal | Astronomy and Astrophysics |
| Volume | 328 |
| Issue number | 2 |
| Publication status | Published - 10 Dec 1997 |
Keywords
- Line: profiles
- Planetary systems
- Stars: circumstellar matter