Models (exercise #0)

The table below organises the data used in each exercise. Data consists in packages compresses with .tar.gz or zip, which can be downloaded by clicking on the provided links.

Data

Package	Date	Author	Description	Format	Download
wp121130_ex0-smodels	21/01/2019	A. Serenelli	stellar interior models	gong, amdl	( ex0-smodels.tar.gz)
wp121130_ex0-omodels	21/01/2019	ALL	oscillations	-	( ex0-frequencies.tar.gz)

Global properties

Model	Mass	[Fe/H]	alpha	Nshell	Phase	Notes
0-001	1.04	+0.05	1.6	3000	MS	Representative of 16Cyg ~7Gyr (Travis et al. 2015)
0-002	1.04	+0.05	1.6	4000	SG	-
0-003	1.50	+0.00	1.6	3000	MS	Small convective core (around 8% of the stellar mass)
0-004	1.50	+0.00	1.6	4000	TAMS	-
0-005	1.50	+0.00	1.6	4000	SG	-

Physics

Relevant constants
Code	Garstec (A- Wess rev., 2015)
Convection	MLT, alpha = 1.801
Overshoot	diffusion equation with exponential decay (Herwig type), including geometric limit applied to small convective cores (H_p towards the center makes overshoot regions too large). Proportion factor f = 0.02 (equivalent to 0.2 - 0.25 Hp in tradicional formulation)
Extra mixing	Under the convective envelope (Vandenberg et al. 2012) as a function of its mass. Free parameters calibration forced to reproduce the solar Li and chemical abundances observed in globular clusters (e.g. Korn et al. en NGC 6397).
gradT	Temperature gradient in overshoot regions is radiative.
Wind	1e-13 Msun / yr to avoid depletion of He and metals (included in extra missing calibration)
Atmosphere	Eddington T-tau
Nuclear rates	Adelberger et al. 2011, which includes de “low” value of LUNA's N14+p
Screening	Weak (Salpeter)/intermediate (Graboske et al. 1973, subgiants)
EOS	FreeEOS de Irwin
Opacities	OPAL + Ferguson 2005 for low temperatures
mDiffusion	For all chemical elements
rLevitation	No
G	6.67232e-8 (c.g.s.)

WP121_130

Table of Contents

Models (exercise #0)

Data

Global properties

Physics