The RADIOSTAR Project

Lugaro, Maria; Côté, Benoit; Pignatari, M.; Yague Lopez, Andres; Brinkman, Hannah; Cseh, Borbála; Den Hartogh, Jacqueline; Doherty, Carolyn; Karakas, Amanda I.; Kobayashi, Chiaki; Lawson, Thomas; Petö, Mária; Soós, Benjámin; Trueman, Thomas; Világos, Blanka

doi:10.3390/universe8020130

Title: The RADIOSTAR Project

Journal Article · 17 February 2022 · Universe

DOI: https://doi.org/10.3390/universe8020130 · OSTI ID:1862816

Lugaro, Maria ^[1]; Côté, Benoit ^[2]; Pignatari, M. ^[3];

^[4]; Brinkman, Hannah ^[5]; Cseh, Borbála ^[6]; Den Hartogh, Jacqueline ^[6]; Doherty, Carolyn ^[6]; Karakas, Amanda I. ^[7]; Kobayashi, Chiaki ^[8]; Lawson, Thomas ^[9]; Petö, Mária ^[6]; Soós, Benjámin ^[10]; Trueman, Thomas ^[9]; Világos, Blanka ^[10]

Konkoly Observatory, Budapest (Hungary). Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH); Eötvös Loránd Univ., Budapest (Hungary). ELTE Inst. of Physics; Monash Univ., Melbourne, VIC (Australia)
Konkoly Observatory, Budapest (Hungary). Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH); Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States). Center for the Evolution of the Elements (JINA-CEE); Univ. of Victoria, BC (Canada)
Konkoly Observatory, Budapest (Hungary). Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH); Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States). Center for the Evolution of the Elements (JINA-CEE); Univ. of Hull (United Kingdom). E.A. Milne Centre for Astrophysics
Konkoly Observatory, Budapest (Hungary). Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Konkoly Observatory, Budapest (Hungary). Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH); Univ. of Szeged (Hungary)
Konkoly Observatory, Budapest (Hungary). Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH)
Monash Univ., Melbourne, VIC (Australia); ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) (Australia)
Univ. of Hertfordshire (United Kingdom). Centre for Astrophysics Research
Konkoly Observatory, Budapest (Hungary). Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH); Univ. of Hull (United Kingdom). E.A. Milne Centre for Astrophysics
Konkoly Observatory, Budapest (Hungary). Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH); Eötvös Loránd Univ., Budapest (Hungary). ELTE Inst. of Physics

Radioactive nuclei are the key to understanding the circumstances of the birth of our Sun because meteoritic analysis has proven that many of them were present at that time. Their origin, however, has been so far elusive. The ERC-CoG-2016 RADIOSTAR project is dedicated to investigating the production of radioactive nuclei by nuclear reactions inside stars, their evolution in the Milky Way Galaxy, and their presence in molecular clouds. So far, we have discovered that: (i) radioactive nuclei produced by $s l o w$ ( $^{107}$ Pd and $^{182}$ Hf) and $r a p i d$ ( $^{129}$ I and $^{247}$ Cm) neutron captures originated from stellar sources —asymptotic giant branch (AGB) stars and compact binary mergers, respectively—within the galactic environment that predated the formation of the molecular cloud where the Sun was born; (ii) the time that elapsed from the birth of the cloud to the birth of the Sun was of the order of 10 $^{7}$ years, and (iii) the abundances of the very short-lived nuclei $^{26}$ Al, $^{36}$ Cl, and $^{41}$ Ca can be explained by massive star winds in single or binary systems, if these winds directly polluted the early Solar System. Our current and future work, as required to finalise the picture of the origin of radioactive nuclei in the Solar System, involves studying the possible origin of radioactive nuclei in the early Solar System from core-collapse supernovae, investigating the production of $^{107}$ Pd in massive star winds, modelling the transport and mixing of radioactive nuclei in the galactic and molecular cloud medium, and calculating the galactic chemical evolution of $^{53}$ Mn and $^{60}$ Fe and of the p-process isotopes $^{92}$ Nb and $^{146}$ Sm.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE; European Research Council (ERC)

Grant/Contract Number:: 89233218CNA000001

OSTI ID:: 1862816

Report Number(s):: LA-UR-22-20334

Journal Information:: Universe, Journal Name: Universe Journal Issue: 2 Vol. 8; ISSN 2218-1997

Publisher:: MDPICopyright Statement

Country of Publication:: United States

Language:: English

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