Index of /~akarakas/model

Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.mso.anu.edu.au/~akarakas/model_data/
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Дата индексирования: Tue Oct 2 00:14:03 2012
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Index of /~akarakas/model_data

 Name                    Last modified      Size  Description
 Parent Directory                             -   
 model_data.files        09-Oct-2007 14:16  323K  
 z0001/                  26-Sep-2007 10:14    -   
 z004/                   26-Sep-2007 10:27    -   
 z008/                   26-Sep-2007 10:31    -   
 z012/                   23-May-2007 17:44    -   
 z02/                    26-Sep-2007 10:36    -

Stellar structure model data during the Asymptotic Giant Branch phase. If you use these
data please provide a reference to the following paper:

Karakas & Lattanzio (2007, PASA, submitted)

Each file contains:

1) pulse number 
2) the core mass, Mcore (Msun)
3) maximum mass of the intershell convection zone, M_csh (Msun)
4) duration of intershell convection, t_csh (years)
5) mass dredged into the envelope, D_dredge (Msun)
6) lambda
7) lambda_dup defined by Goriely & Mowlavi (= lambda x (DMh/Mpulse) where
 	Mpulse is the maximum mass of the intershell convection zone, given in column 2
8) maximum temperature in the He-shell, THeshell (K)
9) maximum temperature at the base of the convective envelope during the
	previous interpulse period, Tbce (K)
10) maximum temperature in the H-shell during the previous interpulse period, THshell (K)
11) interpulse period (years) - note that the first entry is set to zero
12) the total mass, Mtot (Msun)
13) maximum radiated luminosity during the interpulse period, MaxL (Lsun)
14) maximum He-luminosity during a thermal pulse, MaxLHe (Lsun)

All units are in solar units except temperatures, which are in kelvin and
times, which are in years.