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LiBeB, O and Fe Evolution: Refractory Element and Cosmic Ray Transport Delays
Astrophysics · Submitted 18 Jul 2000
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Employing a Monte-Carlo based evolutionary code, we show that the delay of Fe deposition relative to O, due to the incorporation of supernova ejecta refractories in high velocity grains, can account for the rise of [O/Fe] with decreasing [Fe/H].
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The abstract, sentence by sentence
Employing a Monte-Carlo based evolutionary code, we show that the delay of Fe deposition relative to O, due to the incorporation of supernova ejecta refractories in high velocity grains, can account for the rise of [O/Fe] with decreasing [Fe/H]. The predicted behavior of refractory Mg, Si, Ca and Ti, and volatile S, namely that the refractories should not show the rise, but that the behavior of S should be similar to that of O, appears to be confirmed (Takeda et al. 2000, astro-ph/0007007). The delayed deposition of Be, due to cosmic ray transport in a relatively low density medium, leads to consistency of primary Be evolution as a function of both [Fe/H] and [O/H].
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Employing a Monte-Carlo based evolutionary code, we show that the delay of Fe deposition relative to O, due to the incorporation of supernova ejecta refractories in high velocity grains, can account for the rise of [O/Fe] with decreasing [Fe/H]. | result 0.78 | 0.93 | 0.77 | asserted 0.98 |
| s1 | The predicted behavior of refractory Mg, Si, Ca and Ti, and volatile S, namely that the refractories should not show the rise, but that the behavior of S should be similar to that of O, appears to be confirmed (Takeda et al. 2000, astro-ph/0007007). | result 0.86 | 0.16 | 0.08 | asserted 0.53 |
| s2 | The delayed deposition of Be, due to cosmic ray transport in a relatively low density medium, leads to consistency of primary Be evolution as a function of both [Fe/H] and [O/H]. | result 0.85 | 0.80 | 0.19 | asserted 0.88 |
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The paper
Original abstract
Employing a Monte-Carlo based evolutionary code, we show that the delay of Fe deposition relative to O, due to the incorporation of supernova ejecta refractories in high velocity grains, can account for the rise of [O/Fe] with decreasing [Fe/H]. The predicted behavior of refractory Mg, Si, Ca and Ti, and volatile S, namely that the refractories should not show the rise, but that the behavior of S should be similar to that of O, appears to be confirmed (Takeda et al. 2000, astro-ph/0007007). The delayed deposition of Be, due to cosmic ray transport in a relatively low density medium, leads to consistency of primary Be evolution as a function of both [Fe/H] and [O/H].
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