J/ApJS/225/24 NuGrid stellar data set I. Yields from H to Bi (Pignatari+, 2016) ================================================================================ NuGrid stellar data set. I. Stellar yields from H to Bi for stars with metallicities Z=0.02 and Z=0.01. Pignatari M., Herwig F., Hirschi R., Bennett M., Rockefeller G., Fryer C., Timmes F.X., Ritter C., Heger A., Jones S., Battino U., Dotter A., Trappitsch R., Diehl S., Frischknecht U., Hungerford A., Magkotsios G., Travaglio C., Young P. =2016ApJS..225...24P (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Atomic physics ; Models Keywords: nuclear reactions, nucleosynthesis, abundances; stars: abundances stars: evolution; stars: interiors Abstract: We provide a set of stellar evolution and nucleosynthesis calculations that applies established physics assumptions simultaneously to low- and intermediate-mass and massive star models. Our goal is to provide an internally consistent and comprehensive nuclear production and yield database for applications in areas such as presolar grain studies. Our non-rotating models assume convective boundary mixing (CBM) where it has been adopted before. We include 8 (12) initial masses for Z=0.01 (0.02). Models are followed either until the end of the asymptotic giant branch phase or the end of Si burning, complemented by simple analytic core-collapse supernova (SN) models with two options for fallback and shock velocities. The explosions show which pre-SN yields will most strongly be effected by the explosive nucleosynthesis. We discuss how these two explosion parameters impact the light elements and the s and p process. For low- and intermediate-mass models, our stellar yields from H to Bi include the effect of CBM at the He-intershell boundaries and the stellar evolution feedback of the mixing process that produces the ^13^C pocket. All post-processing nucleosynthesis calculations use the same nuclear reaction rate network and nuclear physics input. We provide a discussion of the nuclear production across the entire mass range organized by element group. The entirety of our stellar nucleosynthesis profile and time evolution output are available electronically, and tools to explore the data on the NuGrid VOspace hosted by the Canadian Astronomical Data Centre are introduced. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table9.dat 105 278 The overproduction factors of stable isotopes in stellar winds is given for the stars of Set1.2 table10.dat 55 278 The presupernova overproduction factors of stable isotopes are given for massive stars of Set 1.2 table11.dat 85 278 The isotopic overproduction factors in supernova ejecta is given for the stars of Set 1.2 table12.dat 102 80 The element overproduction factors in stellar winds is given for the stars of Set 1.2 table13.dat 52 80 The presupernova elemental overproduction factors are given for massive stars of Set 1.2 table14.dat 82 80 The elemental overproduction factors in supernova ejecta is given for the stars of Set 1.2 table15.dat 85 278 The overproduction factors of stable isotopes in stellar winds is given for the stars of Set 1.1 table16.dat 35 278 The presupernova overproduction factors of stable isotopes are given for massive stars of Set 1.1 table17.dat 65 278 The overproduction factors of stable isotopes in supernova ejecta is given for the stars of Set 1.1 table18.dat 82 80 The element overproduction factors in stellar winds is given for the stars of Set 1.1 table19.dat 32 80 The presupernova overproduction factors are given for massive stars of Set1.1 table20.dat 62 80 The elemental overproduction factors in supernova ejecta is given for the stars of Set 1.1 -------------------------------------------------------------------------------- See also: J/MNRAS/437/195 : Super and massive AGB stars nucleosynthesis (Doherty+, 2014) J/A+A/560/A16 : Comparison of evolutionary tracks (Martins+, 2013) J/A+A/548/A55 : C & O isotopic ratios in Arcturus and Aldebaran (Abia+ 2012) J/A+A/537/A146 : Stellar models with rotation. 0.8