They planned to do so by carefully calibrating the brightness of a well -
studied type of supernova in very distant galaxies.
Not exact matches
Observations
of type 1a
supernovas imply a faster expansion rate (known as the Hubble constant) than
studies of the cosmic microwave background — light that originated early in cosmic history (SN: 8/6/2016, p. 10).
For this
study, the team set out to investigate the timing
of supernova dust formation by measuring isotopes — versions
of elements with the same number
of protons but different numbers
of neutrons — in rare presolar silicon carbide grains with compositions indicating that they formed in
type II
supernovae.
She accepted an offer from a group
of astronomers at Berkeley, part
of a collaboration
studying a rare
type of supernova that some believe holds the key to measuring the expansion
of the universe.
The evidence for dark energy came from
studies of a kind
of exploding star known as a
Type 1a
supernova.
«We are now fully confident that one
of the most popular
supernova remnants detected in our galaxy was produced by an ordinary
type Ia
supernova that was first detected more than 400 years ago,» write Andrea Pastorello
of Queen's University Belfast and Ferdinando Patat
of the European Southern Observatory in Germany in a commentary on the
study.
These were not included in either Li's or Smartt's
study, both
of which focused on
type II - P
supernovae, the most common
type of core - collapse
supernova.
Neither
study searched for the stars responsible for so - called
type Ia
supernovae, which are explosions
of white dwarf stars that have grown overweight by feasting on material from a companion star.
Type Ia
supernovae are explosions that can be seen even in far - away galaxies and help astronomers
study the large - scale structure
of the Universe.
The standard path to
type Ia
supernovae, the
study's authors wrote, should have produced 30 to 50 times the x-rays observed, indicating that accreting white dwarfs account for less than 5 percent
of the explosions.
The predictable luminosity
of Type Ia
supernovae means that astronomers can use them as cosmic standard candles to measure their distances, making them useful tools in
studying the cosmos.
A group
of astronomers used Hubble to
study the remnant
of the
Type Ia
supernova explosion SNR 0509 - 68.7 — also known as N103B (seen at the top).
But a new
study presents evidence that, for at least one kind
of galaxy, the binary - accretion model should not be more than a minor contributor to the observed
type Ia
supernovae population.
«It will have important repercussions for the
study of supernovae type Ia.»
Other discoveries in the Milky Way detailed in the special edition include the sharpest image yet
of a gamma ray source — a nearby
supernova remnant — which will enable researchers to
study this object at finer scale than before — and three new «gamma ray shells» that are possibly examples
of a new
type of supernova remnant.