Observing
the signature of a single prolific r-process event in
an ultra-faint dwarf galaxy
Anna Frebel (MIT)
The heaviest chemical elements in the periodic table are
synthesized
through the rapid neutron-capture (r-) process but the
astrophysical
site where r-process element nucleosynthesis occurs is still
unknown.
The best candidate sites are ordinary core-collapse
supernovae (deaths of massive stars)
and mergers of two orbiting exotic neutron
stars.
13 billion year old small dwarf galaxies preserve a
"fossil" record of early
chemical enrichment that provides the means to isolate
and study clean
signatures of individual nucleosynthesis events. Based
on new spectroscopic data from the 6.5m Magellan Telescope,
we found
seven stars in the recently discovered dwarf galaxy
Reticulum II that show
extreme overabundances of these heavy r-process
elements.
This "r-process" enhancement implies that the r-process
material in Reticulum II was
synthesized in a single prolific event. Our
results are clearly incompatible
with yield predictions from an ordinary\ core-collapse
supernova but
instead consistent with that of a neutron star merger. This
first signature
of a neutron star merger in the early universe holds the key
to finally,
after 60 years, identifying the cosmic
production site of the r-process.