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.
<Astrophys. J. Suppl. Ser., 225, 24-24 (2016)>
=2016ApJS..225...24P 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 13C
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:
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FileName Lrecl Records Explanations
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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
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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<M<120 (Ekstrom+, 2012)
J/MNRAS/418/284 : s-process in low-metallicity stars. II. (Bisterzo+, 2011)
J/ApJ/726/25 : Production of p-process nuclei in SNe Ia (Kusakabe+, 2011)
J/ApJ/724/975 : Metal-poor star heavy elements abundances (Roederer+, 2010)
J/MNRAS/403/1413 : Updated stellar yields from AGB models (Karakas, 2010)
J/MNRAS/404/1529 : s-process in low-metallicity stars (Bisterzo+, 2010)
J/A+A/512/A10 : Evolution of massive AGB stars. III. (Siess, 2010)
J/A+A/509/A93 : Carbon-enhanced metal-poor stars (Masseron+, 2010)
J/A+A/509/A14 : Grid of solar-metallicity wind models (Mattsson+, 2010)
J/A+A/506/1277 : Magellanic Cloud C/O stars modelisation (Groenewegen+, 2009)
J/ApJ/664/1033 : Variations in supernova yields (Young+ 2007)
J/A+A/441/1195 : Brussels nuclear reaction rate library (Aikawa+, 2005)
J/ApJS/155/651 : Evolution of extremely metal-poor stars (Herwig+, 2004)
J/ApJ/608/405 : Explosive yields of massive star (Chieffi+, 2004)
J/A+A/342/881 : Uncertainties in r-abundance distribution (Goriely 1999)
J/A+AS/96/269 : Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992)
http://nugridstars.org/ : NuGrid project home page
Byte-by-byte Description of file: table9.dat table15.dat
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Bytes Format Units Label Explanations
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1- 5 A5 --- Ion Isotope identifier
7- 15 E9.3 Msun OP1.65 [0.3/9] Overproduction factor for 1.65M☉ model
17- 25 E9.3 Msun OP2 [0.2/34] Overproduction factor for 2M☉ model
27- 35 E9.3 Msun OP3 [0.1/38] Overproduction factor for 3M☉ model
37- 45 E9.3 Msun OP4 [0.01/20] Overproduction factor for 4M☉ model
47- 55 E9.3 Msun OP5 [0.01/9] Overproduction factor for 5M☉ model
57- 65 E9.3 Msun OP15 [0/4] Overproduction factor for 15M☉ model
67- 75 E9.3 Msun OP20 [0/3] Overproduction factor for 20M☉ model
77- 85 E9.3 Msun OP25 [0/4] Overproduction factor for 25M☉ model
87- 95 E9.3 Msun OP32 [0/6]? Overproduction factor for 32M☉ model
(only for table 9)
97-105 E9.3 Msun OP60 [0/59]? Overproduction factor for 60M☉ model
(only for table 9)
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Byte-by-byte Description of file: table1[06].dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 5 A5 --- Ion Isotope identifier
7- 15 E9.3 Msun OP15 [0/223] Overproduction factor for 15M☉ model
17- 25 E9.3 Msun OP20 [0/555] Overproduction factor for 20M☉ model
27- 35 E9.3 Msun OP25 [0/377] Overproduction factor for 25M☉ model
37- 45 A9 Msun OP32 ? Overproduction factor for 32M☉ model
(only for table 10)
47- 55 A9 Msun OP60 ? Overproduction factor for 60M☉ model
(only for table 10)
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Byte-by-byte Description of file: table11.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 5 A5 --- Ion Isotope identifier
7- 15 E9.3 Msun OP15d [0.04/5007] Overproduction factor for 15M☉
delay model
17- 25 E9.3 Msun OP15r [0.04/17490] Overproduction factor for 15M☉
rapid model
27- 35 E9.3 Msun OP20d [0.007/3429] Overproduction factor for 20M☉
delay model
37- 45 E9.3 Msun OP20r [0.007/3359] Overproduction factor for 20M☉
rapid model
47- 55 E9.3 Msun OP25d [0.0003/849] Overproduction factor for 25M☉
delay model
57- 65 E9.3 Msun OP32d [0/10890] Overproduction factor for 32M☉
delay model
67- 75 E9.3 Msun OP32r [0/3400] Overproduction factor for 32M☉
rapid model
77- 85 E9.3 Msun OP60d [0/2722] Overproduction factor for 60M☉
delay model
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Byte-by-byte Description of file: table1[28].dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- Sp Species identifier
4- 12 E9.3 Msun OP1.65 [0/3] Overproduction factor for 1.65M☉ model
14- 22 E9.3 Msun OP2 [0/8] Overproduction factor for 2M☉ model
24- 32 E9.3 Msun OP3 [0/8] Overproduction factor for 3M☉ model
34- 42 E9.3 Msun OP4 [0/10] Overproduction factor for 4M☉ model
44- 52 E9.3 Msun OP5 [0/5] Overproduction factor for 5M☉ model
54- 62 E9.3 Msun OP15 [0/3] Overproduction factor for 15M☉ model
64- 72 E9.3 Msun OP20 [0/3] Overproduction factor for 20M☉ model
74- 82 E9.3 Msun OP25 [0/4] Overproduction factor for 25M☉ model
84- 92 E9.3 Msun OP32 [0/6]? Overproduction factor for 32M☉ model
(only for table 12)
94-102 E9.3 Msun OP60 [0/19]? Overproduction factor for 60M☉ model
(only for table 12)
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Byte-by-byte Description of file: table1[39].dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- Sp Species identifier
4- 12 E9.3 Msun OP15 [0/33] Overproduction factor for 15M☉ model
14- 22 E9.3 Msun OP20 [0/40] Overproduction factor for 20M☉ model
24- 32 E9.3 Msun OP25 [0/31] Overproduction factor for 25M☉ model
34- 42 E9.3 Msun OP32 [0/49]? Overproduction factor for 32M☉ model
(only for table 13)
44- 52 E9.3 Msun OP60 [0/225]? Overproduction factor for 60M☉ model
(only for table 13)
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Byte-by-byte Description of file: table14.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- Sp Species identifier
4- 12 E9.3 Msun OP15d [0/1182] Overproduction factor for 15M☉
delay model
14- 22 E9.3 Msun OP15r [0/3410] Overproduction factor for 15M☉
rapid model
24- 32 E9.3 Msun OP20d [0/99] Overproduction factor for 20M☉
delay model
34- 42 E9.3 Msun OP20r [0/99] Overproduction factor for 20M☉
rapid model
44- 52 E9.3 Msun OP25d [0/52] Overproduction factor for 25M☉
delay model
54- 62 E9.3 Msun OP32d [0/1815] Overproduction factor for 32M☉
delay model
64- 72 E9.3 Msun OP32r [0/262] Overproduction factor for 32M☉
rapid model
74- 82 E9.3 Msun OP60d [0/338] Overproduction factor for 60M☉
delay model
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table17.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 5 A5 --- Ion Isotope identifier
7- 15 E9.3 Msun OP15d [0.01/19420] Overproduction factor for 15M☉
delay model
17- 25 E9.3 Msun OP15r [0.01/80590] Overproduction factor for 15M☉
rapid model
27- 35 E9.3 Msun OP20d [0.001/1176] Overproduction factor for 20M☉
delay model
37- 45 E9.3 Msun OP20r [0.001/1428] Overproduction factor for 20M☉
rapid model
47- 55 E9.3 Msun OP25d [0.0007/1093] Overproduction factor for 25M☉
delay model
57- 65 E9.3 Msun OP25r [0/46] Overproduction factor for 25M☉
rapid model
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table20.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- Sp Species identifier
4- 12 E9.3 Msun OP15d [0/3684] Overproduction factor for 15M☉
delay model
14- 22 E9.3 Msun OP15r [0/21690] Overproduction factor for 15M☉
rapid model
24- 32 E9.3 Msun OP20d [0/117] Overproduction factor for 20M☉
delay model
34- 42 E9.3 Msun OP20r [0/678] Overproduction factor for 20M☉
rapid model
44- 52 E9.3 Msun OP25d [0/57] Overproduction factor for 25M☉
delay model
54- 62 E9.3 Msun OP25r [0/9] Overproduction factor for 25M☉
rapid model
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History:
From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 13-Oct-2016