Not exact matches
«The fact that this
supernova event didn't expel the
other star, which is 20 to 25 times the mass
of our sun, makes this an incredibly rare
type of binary system.»
• How might the burned - out stars called white dwarfs be brought to ruin by
other stars in so - called
Type Ia
supernovae, inciting the fiery alchemy that yielded much
of the iron in our blood and the potassium in our brains?
In fact, SN 2017egm was not only superluminous, but superclose: At just 420 million light - years away, it was three times closer than any
other observed
supernova of its
type.
The Hubble Space Telescope's recent discovery
of the earliest known
Type Ia
supernova from more than 10 billion years ago, plus
other results, favor a scenario in which two white dwarfs merge.
Other telescopes around the world soon confirmed that it was a
type Ia
supernova, one
of the brightest events
of the cosmos.
To check the value
of the Hubble constant that they have obtained from a single object, Schmidt and his colleagues plan to apply their technique to
other type II
supernovae that have occurred in distant galaxies.
Type Ia
supernovae completely destroy the core
of a star, but the
other three
types leave a super-dense core behind.
It's so consistent that
Type Ia
supernovae are also called standard candles: Once astronomers find one in a region
of space, they can use it as a baseline with which to compare
other objects around it.
Before 1987, astronomers believed that only red supergiants would explode as
supernovae, but this observation proved that
other types of evolved stars can produce these explosions too.
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.
Optical and near - infrared coverage
of SN 2004et: physical parameters and comparison with
other type IIP
supernovae.
They applied a new technique that could have implications for understanding
other Type Ia
supernovae, a class
of stellar explosions that scientists use to determine the expansion rate
of the universe.
Using Keck, we have traced atoms as they flow from the intergalactic medium into galaxies, where they are incorporated into stars, undergo fusion, and are returned in
supernovae and
other types of stellar death.