Steady-state nucleosynthesis throughout the Galaxy

Abstract

Measurement and astrophysical interpretation of characteristic gamma-ray lines from nucleosynthesis was one of the prominent science goals of the INTEGRAL mission and in particular its spectrometer SPI. Emission from 26Al and from 60Fe decay lines originates from accumulated ejecta of nucleosynthesis sources, and appears diffuse in nature. 26Al and 60Fe are believed to originate mostly from massive star clusters. Gamma-ray observations open an interesting window to trace the fate and flow of nucleosynthesis ejecta, after they have left the immediate sources and their birth sites, and on their path to mix with ambient interstellar gas. The INTEGRAL 26Al emission image confirms earlier findings of clumpiness and an extent along the entire plane of the Galaxy, supporting its origin from massive-star groups. INTEGRAL spectroscopy resolved the line and found Doppler broadenings and systematic shifts from large-scale galactic rotation. But an excess velocity of ~200 km/s suggests that 26Al decays preferentially within large superbubbles that extend in forward directions between spiral arms. The detection of 26Al line emission from nearby Orion and the Eridanus superbubble supports this interpretation. Positrons from beta+ decays of 26Al and other nucleosynthesis ejecta have been found to not explain the morphology of positron annihilation gamma-rays at 511 keV that have been measured by INTEGRAL. The 60Fe signal measured by INTEGRAL is diffuse but too weak for an imaging interpretation, an origin from point-like/concentrated sources is excluded. The 60Fe/26Al ratio is constrained to a range 0.2-0.4. Beyond improving precision of these results, diffuse nucleosynthesis contributions from novae (through 22Na radioactivity) and from past neutron star mergers in our Galaxy (from r-process radioactivity) are exciting new prospects for the remaining mission extensions.

38 pages, 12 Figures. Contribution to Review Book "15 years of INTEGRAL". Accepted for publication in New Astronomy Reviews

References in corpus (14)

• Physical Properties of Wolf-Rayet Stars
• The Dawes Review 2: Nucleosynthesis and stellar yields of low and intermediate-mass single stars
• The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
• Stellar Models and Yields of Asymptotic Giant Branch Stars
• Dawes Review 4: Spiral Structures in Disc Galaxies
• The Galactic ${}^{26}$Al emission map as revealed by INTEGRAL/SPI
• 26Al kinematics: superbubbles following the spiral arms? Constraints from the statistics of star clusters and HI supershells
• Gamma-ray Emission of 60Fe and 26Al Radioactivities in our Galaxy
• Triggered Star Formation on the Border of the Orion-Eridanus Superbubble
• Dynamics and Energy Loss in Superbubbles
• Comparing simulated ${}^{26}$Al maps to gamma-ray measurements
• Synthetic ${}^{26}$Al emission from galactic-scale superbubble simulations
• Squeezed between shells? On the origin of the Lupus I molecular cloud. - II. APEX CO and GASS HI observations
• SPI/INTEGRAL observation of 1809 keV gamma-ray line emission from the Cygnus X region

Cited by in corpus (7)

• Measurement of Galactic ${}^{26}$Al with the Compton Spectrometer and Imager
• Gamma-Ray Light Curves and Spectra of Classical Novae
• Radioactive isotopes in the interstellar medium
• Cosmic Radioactivity and Galactic Chemical Evolution
• Nuclear astrophysics
• A New Versatile Code for Gamma-Ray Monte-Carlo Radiative Transfer
• Gamma-ray spectroscopy of galactic nucleosynthesis