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Astrophysical Journal Letters, ISSN 2041-8205, 02/2017, Volume 835, Issue 2, pp. L26 - 26
A new analysis of cosmic ray (CR) data collected by the SOKOL experiment in space found that the deuteron-to-helium ratio at energies between 500 and 2000... 
ISM: supernova remnants | cosmic rays | acceleration of particles | nuclear reactions nucleosynthesis abundances | ORIGIN | nucleosynthesis | NUCLEI | abundances | ASTRONOMY & ASTROPHYSICS | nuclear reactions | PROPAGATION | Supernova remnants | Deuterons | Chromium | Nucleons | Isotopes | Joints | Interstellar matter | Cosmic rays
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 12/2001, Volume 563, Issue 1, pp. 185 - 190
Among the many new nuclei synthesized in supernova explosions are unstable proton-rich isotopes. Many of these decay by electron capture, leaving atomic... 
Supernovae: general | Nuclear reactions, nucleosynthesis, abundances | Supernova remnants | X-rays: general | nuclear reactions, nucleosynthesis, abundances supernova remnants | X-rays : general | LINE EMISSION | DISTANCE | ASTRONOMY & ASTROPHYSICS | TI-44 | CONSTRAINTS | SOLAR-SYSTEM | SN 1987A | supernovae : general
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 01/2003, Volume 582, Issue 1, pp. 257 - 261
Two long observations of the Cas A supernova remnant were made by the Rossi X-Ray Timing Explorer in 1996 and 1997 to search for hard X-ray line emission at... 
nuclear reactions, nucleosynthesis, abundances supernova remnants | X-rays : individual (Cassiopeia A) | HALF-LIFE | SHELL | MODELS | ELECTRONS | ASTRONOMY & ASTROPHYSICS | CAS-A | EXPLOSION | STARS | EMISSION | A SUPERNOVA REMNANT
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 10/1999, Volume 524, Issue 1, pp. 213 - 219
We estimate gamma-ray fluxes due to the decay of nuclei beyond Bi-209 from a supernova or a supernova remnant assuming that the r-process occurs in supernovae.... 
nuclear reactions, nucleosynthesis, abundances supernova remnants | ELEMENTS | DIVERSE SUPERNOVA SOURCES | ASTRONOMY & ASTROPHYSICS | SOLAR | METAL-POOR | CS-22892-052 | STARS | gamma rays : theory | INTERSTELLAR-MEDIUM | ABUNDANCES | supernovae : general
Journal Article
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 03/2015, Volume 801, Issue 2, pp. L31 - 6
Journal Article
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 05/2019, Volume 485, Issue 3, pp. 4287 - 4310
We investigate 60Fe in massive stars and core-collapse supernovae focussing on uncertainties that influence its production in 15, 20 and 25 M⊙ stars at solar... 
nucleosynthesis | massive | abundances | ASTRONOMY AND ASTROPHYSICS | nuclear reactions | stars: abundances | supernovae: general | gamma-rays: stars
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2018, Volume 856, Issue 1, p. 63
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 09/2019, Volume 629, p. A51
Magnetars are regarded as the most magnetized neutron stars in the Universe. Aiming to unveil what kinds of stars and supernovae can create magnetars, we have... 
MASSIVE STARS | ISM: supernova remnants | nuclear reactions, nucleosynthesis, abundances | stars: magnetars | pulsars: general | NEUTRON-STAR | PULSAR | EVOLUTION | PROGENITOR | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | NUCLEOSYNTHESIS | EMISSION
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 05/2019, Volume 485, Issue 3, pp. 4287 - 4310
We investigate Fe-60 in massive stars and core-collapse supernovae focussing on uncertainties that influence its production in 15, 20, and 25 M-circle dot... 
WEAK INTERACTION RATES | nuclear reactions, nucleosynthesis, abundances | NUCLEAR | RADIOACTIVE AL-26 | TRIPLE-ALPHA | MASS-LOSS RATES | stars: abundances | supernovae: general | EVOLUTION | ASTRONOMY & ASTROPHYSICS | STARS | SOLAR-SYSTEM | NUCLEOSYNTHESIS | gamma-rays: stars | M-CIRCLE-DOT
Journal Article