Nucleosynthesis in Stars and the Chemical Enrichment of Galaxies

By Ken'ichi Nomoto, C. Kobayashi, Nozomu Tominaga. 2013

728 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/256ca2e1c8514d16c780c224a26794671ed24310

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Stan Woosley
2. Hans-Thomas Janka
3. S. Smartt
4. N. Langer
5. A. Karakas
6. B. Metzger
7. Michela Mapelli
8. N. Smith

In Instrumentation

1. A. Karakas
2. M. Lugaro
3. Stan Woosley
4. N. Langer
5. Weidong Li
6. N. Smith
7. A. Chieffi
8. M. Limongi

Citations in the corpus

• CORE-COLLAPSE SUPERNOVAE FROM 9 TO 120 SOLAR MASSES BASED ON NEUTRINO-POWERED EXPLOSIONS (2015, background): “The study of nucleosynthesis in massive stars has a rich history (e.g., Burbidge et al. 1957; Woosley & Weaver 1995; Thielemann et al. 1996; Woosley et al. 2002; Nomoto et al. 2013).”
• TOWARD CHARACTERIZATION OF THE TYPE IIP SUPERNOVA PROGENITOR POPULATION: A STATISTICAL SAMPLE OF LIGHT CURVES FROM Pan-STARRS1 (2014, background): “…to and constraint on models of stellar evolution for massive stars (Groh et al. 2013a; Meynet et al. 2013), chemical evolution (Timmes et al. 1995; Nomoto et al. 2006, 2013), supernova feedback in the interstellar medium and galaxy formation (Leitherer et al. 1992; Stilp et al. 2013), and…”
• THE MASS SPECTRUM OF THE FIRST STARS (2014, methodology): “We find that the yield of the heavy elements that is obtained by integrating the mass spectrum is not consistent with that of the low metallicity DLA systems/EMP stars, because the fraction of PISNe is too large.”
• Chemical evolution with rotating massive star yields - I. The solar neighbourhood and the s-process elements (2018, methodology): “To explain the behavior of both Cu and Zn at low metallicities, specific models have been suggested, invoking simultaneously: inhomogeneous early chemical evolution, a large fraction of hypernova at low metallicities (∼ 50% of stars with M> 2 M ) and a peculiar mechanism of ”mixing and fallback” of ”
• Origin of the heaviest elements: The rapid neutron-capture process (2019, background): “These basic features of galactic evolution have been understood reasonably well for the majority of elements (Matteucci and Greggio, 1986; Timmes et al., 1995; Nomoto et al., 2013), while open questions remain in stellar evolution and supernova explosion mechanisms.”
• STELLAR YIELDS FROM METAL-RICH ASYMPTOTIC GIANT BRANCH MODELS (2016, background): “Stellar yields are an essential ingredient for theoretical calculations of Galactic chemical evolution (Tinsley 1980; Romano et al. 2010; Nomoto et al. 2013; Karakas & Lattanzio 2014; Mollá et al. 2015).”
• The Intermediate r-process in Core-collapse Supernovae Driven by the Magneto-rotational Instability (2016, result): “These values are comparable to those for HNe (see, a resent review, Nomoto et al. 2013).”
• The Carnegie Supernova Project. I. Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions (2017, background): “TypeIa SNe are important for their role in the chemical enrichment of the universe (e.g., Nomoto et al. 2013, and references therein).”
• MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS (2015, background): “There are many ways M & 8 M stars can end their lives 3 (e.g., Woosley et al. 2002; Smartt 2009; Meynet et al. 2010; Langer 2012; Nomoto et al. 2013; Smith 2014).”
• Neutron Star Mergers Might Not Be the Only Source of r-process Elements in the Milky Way (2018, methodology): “…properties of different enrichment sites, GCE simulations also take into account galaxy evolution processes such as star formation and interactions between galaxies and their surrounding medium (e.g., Gibson et al. 2003; Prantzos 2008; Nomoto et al. 2013; Matteucci 2014; Somerville & Davé 2015).”