Yunnan Models

for CSPs

 

1. Brief description: Yunnan-II models for CSPs

Based on Yunnan-II-BaSeL (models with and without BIs) and Yunnan-II-BaSeL-sdB (models with BIs) models, we present the ISEDs of E, S0, Sa-Sd, Irr galaxies and the ISEDs of galaxies with short e-folding timescales by advantage of a ¦Ä-form, six exponentially decreasing (timescale = 1, 2, 3, 5, 15 and 30Gyr), a constant-form and five exponentially decreasing (timescale ¦Ó = 0.1, 0.3, 0.5, 0.7 and 0.9Gyr) SFRs. Age (90): from 1.e+6 to 1.5e+10 yr. Metallicity (7): from 1.e-4 to 0.03.

The data of 8 galaxy types ( E, S0, Sa-Sd and Irr) at solar metallicity have even been used in our papers (2010.MNRAS.408.1283; 2012.MNRAS.421.743; 2010.Ap&SS.329.249), those of the other 5 galaxy types at solar metallicity and all galaxy types at non-solar metallicity have not been used and published before.

2. Download region

CSPs with and without BIs

(Yunnan-II-BaSeL)
ISEDs

Download, READTB.f, 182 files

 solar-Z: this website (NEW!)

8 galaxy types: used in 2010.MNRAS.408.1283 & 2012.MNRAS.421.743

the other 5 types: and not been used

other-Z: this website (NEW!)

8 galaxy types: used in 2013.MN.preparation the other 5 types: and not been used

CSPs with BIs

(Yunnan-II-BaSeL-sdB)
ISEDs

Download, READTB.f, 91 files

 solar-Z: this website (NEW!)

8 galaxy types: used in 2010.Ap&SS.329.249 the other 5 types: and not been used
other-Z: this website (NEW!) and not been used

 
 

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