Evolutionary Synthesis Models
Dispersion and spectrum
Welcome to SED@: evolutionary synthesis models for young star forming regions that compute the Stellar Energy Dispersion and Distribution and are available on the WWW (@).
We hope that this server will be useful for you
We had updated the code by Cerviño & Mas-Hesse (1994) to include an estimation of the dispersion and confidence levels of the different observables. We show here the results of the observables computed by the code. We have not tested all of then so if you find something strange, please, help us to improve the code an say us (send a mail to email@example.com). If you are interested in any other observable, please contact us.
Here you can access to:
- The History of the models.
- Some Theory about them
- Other servers with synthesis models and related issues
- Database Output results of models for all the set of tracks; all computed with the Geneva evolutionary tracks.
- Currently, we are working on an update of the code, that will we written in ANSI-C and will be available to the community (together with complete manuals) during 2003 (tentative date).
If you want the results from 26Al and 60Fe gamma-ray lines:
Click here to access to the output tables used in Cerviño et al. 2000 A&A 363, 970
If you want Access to Cerviño & Mas-Hesse (1994, A&A 284, 749) models,Please, contact us.Miguel Cerviño
Justicia, no venganza|
Justice, not revenge
We thanks to the LAEFF for the space for host this server