Gamma-ray line emission from radioactive isotopes in stars and galaxies

Roland Diehl, Francis Timmes

Research output: Contribution to journalArticle

86 Citations (Scopus)

Abstract

Our modern laboratory of nuclear physics has expanded to encompass parts of the universe, or at least our Galaxy. Gamma rays emitted by the decays of radioactive nuclei testify to the production of isotopes through nuclear processes in astrophysical events. We collect measurements of the Galactic γ-ray sky in spectral lines attributed to the decay of radioactive 7Be, 22Na, 26Al, 44Ti, 56Ni, 57Ni, and 60Fe. We organize and collate these measurements with models for the production sites in novae, supernovae, stellar interiors, and interstellar cosmic-ray interactions. We discuss the physical processes and the spatial distribution of these production sites, along with models of the chemical evolution of the Galaxy. Highlights of measurements made in the last decade include detailed images of the Galaxy in 26Al radioactivity and detection of 56Co and 57Co from SN 1987A, 44Ti from Cas A, and possibly 56Ni from SN 1991T. The 26Al mapping of recent Galactic nucleosynthesis may be considered as a new view on the entire ensemble of massive stars in the Galaxy. The local Cygnus region shows prominent radioactive emission from well-known stellar clusters, but the absence of γ-rays from the closest Wolf-Rayet star, WR 11, in the Vela region is puzzling. SN 1987A studies in γ-rays measure the radioactive powering of the supernova light curve directly, which will be particularly important for the dim late phase powered by 44Ti. The 57Ni/56Ni isotopic ratio determinations from γ-rays provide additional guidance for understanding SN 1987A's complex light curve and now appear to be uniformly settling to about twice the solar ratio. Cas A 44Ti production as measured through γ-rays presents the interesting puzzle of hiding the expected, coproduced, and large 56Ni radioactivity. Core-collapse supernova models need to parameterize the inner boundary conditions of the supernova in one way or another, and now enjoy another measurement of the ejecta that is definitely originating from very close to the difficult regime of the mass cut between ejecta and compact remnant. Other relevant measurements of cosmic element abundances, such as observations of atomic lines from the outer shells of the production sites or meteoritic analysis of interstellar grains, complement the rather direct measurements of penetrating γ-rays, thus enhancing the observational constraints of nuclear astrophysics models.

Original languageEnglish (US)
Pages (from-to)637-659
Number of pages23
JournalPublications of the Astronomical Society of the Pacific
Volume110
Issue number748
StatePublished - Jun 1998
Externally publishedYes

Fingerprint

radioactive isotopes
gamma rays
rays
isotope
galaxies
stars
supernovae
ejecta
radioactivity
astrophysics
light curve
isotopic ratio
cosmic ray
boundary condition
stellar interiors
nuclear astrophysics
novae
Wolf-Rayet stars
shell
spatial distribution

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Gamma-ray line emission from radioactive isotopes in stars and galaxies. / Diehl, Roland; Timmes, Francis.

In: Publications of the Astronomical Society of the Pacific, Vol. 110, No. 748, 06.1998, p. 637-659.

Research output: Contribution to journalArticle

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