grad course lecture at U. Padova

The optically thick wind theory and it's application 

 
No1. (10/10)

  1. introduction of nova

  2. Eddington luminosity and occurrence of the winds

  3. OPAL opacity
-----------------------------------------
No2. (10/17)

4. shell flash

5. theoretical work of shell flash

6. composition of nova ejecta

7. Optically thick wind theory

8. speed class of nova and whithe dwarf mass
-----------------------------------------
No3. (10/24)

9. optical, UV and X-ray from nova

10. Universal decline law of nova light curves

11. light curve analysis of nova -- how to detemine the WD mass

12. light curve analysis of classical novae 

13. light curve analysis of recurrent novae
---------------------------------------------
No4. (10/30)

14. He nova

15. V445 Pup

16. accretion wind evolution

17. RX J0513-69 and  V Sge

----------------------------------------------
No5. (11/7)

18. Supernova I and II

19. Introduction of binary evolution

20. double degenerate(DD) and single degenerate (SD)
   scenarios to type Ia SN

21. acccretion wind evolution

22. SSS channel and symbiotic channel

23. corresponding progenitors

24. formation of circumstellar matter
   and recent observation of CSM of SN Ia