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100527e19850101||| s| f1|||||eng|d |
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|a (TOE)ost5351849
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|a (TOE)5351849
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|a TOE
|c TOE
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|a GDWR
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|a 71
|2 edbsc
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|a E 1.99: conf-850375-19
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|a E 1.99:ucrl-92972
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| 086 |
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|a E 1.99: conf-850375-19
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| 245 |
0 |
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|a Theoretical models for Type I and Type II supernova
|h [electronic resource]
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| 260 |
|
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|a Oak Ridge, Tenn. :
|b distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy,
|c 1985.
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| 300 |
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|a Pages: 28 :
|b digital, PDF file.
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| 336 |
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|a text
|b txt
|2 rdacontent.
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| 337 |
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|a computer
|b c
|2 rdamedia.
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| 338 |
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|a online resource
|b cr
|2 rdacarrier.
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| 500 |
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|a Published through the Information Bridge: DOE Scientific and Technical Information.
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| 500 |
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|a 01/01/1985.
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|a "ucrl-92972"
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|a " conf-850375-19"
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| 500 |
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|a "DE85016288"
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| 500 |
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|a 20. Recontre de Moriond, Les Arcs, France, 10 Mar 1985.
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| 500 |
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|a Weaver, T.A.; Woosley, S.E.
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| 500 |
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|a California Univ., Santa Cruz (USA). Lick Observatory.
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| 520 |
3 |
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|a Recent theoretical progress in understanding the origin and nature of Type I and Type II supernovae is discussed. New Type II presupernova models characterized by a variety of iron core masses at the time of collapse are presented and the sensitivity to the reaction rate ¹²C(..cap alpha..,..gamma..)¹⁶O explained. Stars heavier than about 20 M/sub solar/ must explode by a ''delayed'' mechanism not directly related to the hydrodynamical core bounce and a subset is likely to leave black hole remnants. The isotopic nucleosynthesis expected from these massive stellar explosions is in striking agreement with the sun. Type I supernovae result when an accreting white dwarf undergoes a thermonuclear explosion. The critical role of the velocity of the deflagration front in determining the light curve, spectrum, and, especially, isotopic nucleosynthesis in these models is explored. 76 refs., 8 figs.
|
| 536 |
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|b W-7405-ENG-48.
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| 650 |
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7 |
|a Information.
|2 local.
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| 650 |
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7 |
|a Thermodynamic Model.
|2 local.
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| 650 |
|
7 |
|a Hydrodynamic Model.
|2 local.
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| 650 |
|
7 |
|a Chemical Composition.
|2 local.
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| 650 |
|
7 |
|a Numerical Data.
|2 local.
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| 650 |
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7 |
|a Mathematical Models.
|2 local.
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| 650 |
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7 |
|a White Dwarf Stars.
|2 local.
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| 650 |
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7 |
|a Supernovae.
|2 local.
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| 650 |
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7 |
|a Synthesis.
|2 local.
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| 650 |
|
7 |
|a Nucleosynthesis.
|2 local.
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| 650 |
|
7 |
|a Statistical Models.
|2 local.
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| 650 |
|
7 |
|a Origin.
|2 local.
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| 650 |
|
7 |
|a Theoretical Data.
|2 local.
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| 650 |
|
7 |
|a Stars.
|2 local.
|
| 650 |
|
7 |
|a Star Evolution.
|2 local.
|
| 650 |
|
7 |
|a Eruptive Variable Stars.
|2 local.
|
| 650 |
|
7 |
|a Particle Models.
|2 local.
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| 650 |
|
7 |
|a Data.
|2 local.
|
| 650 |
|
7 |
|a Dwarf Stars.
|2 local.
|
| 650 |
|
7 |
|a Variable Stars.
|2 local.
|
| 650 |
|
7 |
|a Black Holes.
|2 local.
|
| 650 |
|
7 |
|a Classical And Quantum Mechanics, General Physics.
|2 edbsc.
|
| 710 |
2 |
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|a Lawrence Livermore National Laboratory.
|4 res.
|
| 710 |
1 |
|
|a United States.
|b Department of Energy.
|b Office of Scientific and Technical Information.
|4 dst.
|
| 856 |
4 |
0 |
|u http://www.osti.gov/servlets/purl/5351849-ClfO3O/
|z Online Access
|
| 907 |
|
|
|a .b60068747
|b 03-06-23
|c 05-30-10
|
| 998 |
|
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|a web
|b 05-30-10
|c f
|d m
|e p
|f eng
|g
|h 0
|i 1
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| 956 |
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|a Information bridge
|
| 999 |
f |
f |
|i 8007e522-f84f-55be-9852-506f0b734c65
|s 2f632f10-9c81-5a91-8f52-108e8ed17a43
|
| 952 |
f |
f |
|p Can circulate
|a University of Colorado Boulder
|b Online
|c Online
|d Online
|e E 1.99: conf-850375-19
|h Superintendent of Documents classification
|i web
|n 1
|
