SpS5 - II. Stellar and wind parameters
Overview & Synopsis
The development of infrared observational facilities has revealed a number of massive stars in obscured environments throughout the Milky Way and beyond. The determination of their stellar and wind properties from infrared diagnostics is thus required to take full advantage of the wealth of observations available in the near and mid infrared. However, the task is challenging. This session addressed some of the problems encountered and showed the limitations and successes of infrared studies of massive stars.
Indexed from repository: HAL Open Science
(
hal.science)
Keyboard Shortcuts:
← / → for pages • + / - for zoom • 0 to fit width
Powered by Mozilla PDF.js v3.11
Document Information
| Document Title | SpS5 - II. Stellar and wind parameters |
|---|---|
| Author / Organization | Fabrice Martins, M. Bergemann, J.M. Bestenlehner, P.A. Crowther, W.R. Hamann, F. Najarro, M.F. Nieva, N. Przybilla, J. Freimanis, W. Hou, L. Kaper, C.-D. Lee |
| Subject & Discipline | Multidisciplinary Academic Open Research |
| Categories | Science & Mathematics |
| Publication Year | 2012 |
| License / Rights | Open Access / Creative Commons |
| Resource Verification | Listed PDF (Verification Pending) |
| Original Host Website |
HAL Open Science
(hal.science)
|
| File Format | application/pdf (Portable Document Format) |
| Language | EN |
| Catalog ID | DOC-120022 |
| Original Source Link | Visit Source Page on hal.science » |