A Test of the Supernova Trigger Hypothesis with [TSUP]60[/TSUP]F[CLC]e[/CLC] and [TSUP]26[/TSUP]A[CLC]l[/CLC]
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference40 articles.
1. The late behavior of supernova 1987A. I - The light curve. II - Gamma-ray transparency of the ejecta
2. Carbon-Burning Nucleosynthesis at Constant Temperature
3. On the Production of [TSUP]26[/TSUP]Al in the Early Solar System by Low-Energy Oxygen Cosmic Rays
4. Evidence for the presence of53Mn in the early solar system
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1. Limits on Supernova-Associated Fe60/Al26 Nucleosynthesis Ratios from Accelerator Mass Spectrometry Measurements of Deep-Sea Sediments;Physical Review Letters;2018-11-27
2. On the Origin of Early Solar System Radioactivities: Problems with the Asymptotic Giant Branch and Massive Star Scenarios;The Astrophysical Journal;2018-08-16
3. Short-lived radioactivities in the early solar system: A fossil record of our origins in stars;The European Physical Journal Plus;2018-07
4. New Constraints on the Abundance of 60 Fe in the Early Solar System;The Astrophysical Journal;2018-04-19
5. The Early Solar System;Astrophysics with Radioactive Isotopes;2018
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