Abstract
The study of the structure of our Galaxy requires to determine the distance of young objects (especially O and B stars). We review the method used and the main results of our study of the large scale structure of our Galaxy before presenting the potential improvements of the Gaia data.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 191-192 |
| Number of pages | 2 |
| Journal | European Space Agency, (Special Publication) ESA SP |
| Issue number | 576 |
| State | Published - Aug 22 2005 |
| Externally published | Yes |
| Event | Symposium - The Three-Dimensional Universe with Gaia - Paris, France Duration: Oct 4 2004 → Oct 7 2004 |
Keywords
- Galaxy: structure
- Young stars
ASJC Scopus subject areas
- Aerospace Engineering
- Space and Planetary Science