A team of European astronomers using ESO's Very Large Telescope (VLT) now believe they've found the partner
star of a magnetar for the first time.
Not exact matches
Of about 2,600 neutron
stars known, to date only 29 are classified as
magnetars.
Astronomers have discovered a vast cloud
of high - energy particles called a wind nebula around a rare ultra-magnetic neutron
star, or
magnetar, for the first time.
Two common models for gamma - ray emission from FRBs exist: one invoking magnetic flare events from
magnetars — highly magnetized neutron
stars that are the dense remnants
of collapsed
stars — and another invoking the catastrophic merger
of two neutron
stars, colliding to form a black hole.
Some, for reasons that are not totally understood, fall under the classification
of «
magnetars,» which take the already - astounding field
of an ordinary neutron
star and multiply it by about 1,000 times.
In the first stage
of this process, the more massive
star of the pair begins to run out
of fuel, transferring its outer layers to its less massive companion — which is destined to become the
magnetar — causing it to rotate more and more quickly.
The discovery
of the
magnetar's former companion elsewhere in the cluster helps solve the mystery
of how a
star that started off so massive could become a
magnetar, rather than collapse into a black hole.
The rapid rotation created by mass transfer between the two
stars appears necessary to generate the ultra-strong magnetic field and then a second mass transfer phase allows the
magnetar - to - be to slim down sufficiently so that it does not collapse into a black hole at the moment
of its death.
They hunted for runaway
stars — objects escaping the cluster at high velocities — that might have been kicked out
of orbit by the supernova explosion that formed the
magnetar.
Extremely bright exploding
stars, called superluminous supernovae, and long gamma ray bursts also occur in this type
of galaxy, he noted, and both are hypothesized to be associated with massive, highly magnetic and rapidly rotating neutron
stars called
magnetars.
They suggested that the
magnetar formed through the interactions
of two very massive
stars orbiting one another in a binary system so compact that it would fit within the orbit
of the Earth around the Sun.
The Westerlund 1
star cluster [1], located 16,000 light - years away in the southern constellation
of Ara (the Altar), hosts one
of the two dozen
magnetars known in the Milky Way.
The new study finds that the supernovae are likely powered by the creation
of a
magnetar, an extraordinarily magnetized neutron
star spinning hundreds
of times per second.
Magnetars have the mass
of the sun packed into a
star the size
of a city and have magnetic fields a hundred trillion times that
of Earth.
They also discovered a new
magnetar, a rare kind
of neutron
star (a
star as dense as an atomic nucleus but the size
of a city).
The characteristics
of the surrounding
stars suggest that although the
magnetar's progenitor probably reached 40 solar masses at one point, it shed its mass so quickly that when the
star exploded it fell under the 20 - solar - mass limit, thereby creating a
magnetar instead
of a black hole — and conforming to current theory about stellar evolution.
Like all
magnetars, CXOU J164710.2 - 455216 is a rare kind
of neutron
star that for as - yet - unexplained reasons possesses the most powerful magnetic field in the universe.
Yet according to detailed measurements
of the relative motions
of the surrounding
stars, the team reports in an upcoming issue
of Astronomy & Astrophysics, that like every neighboring
star, the mass
of the
magnetar's progenitor must have been at least 40 times greater than the sun's.
The Dutch and Breakthrough Listen teams suggest that the fast radio bursts may come from a highly magnetized rotating neutron
star — a
magnetar — in the vicinity
of a massive black hole that is still growing as gas and dust fall into it.
Thornton, however, favours
magnetars — highly magnetic neutron
stars — as the source
of FRBs.
Magnetars have the mass
of the sun packed into a
star the size
of a city and have magnetic fields a hundred trillion times that
of the Earth.
The top candidates, the astronomers suggested, are a neutron
star, possibly a highly - magnetic
magnetar, surrounded by either material ejected by a supernova explosion or material ejected by a resulting pulsar, or an active nucleus in the galaxy, with radio emission coming from jets
of material emitted from the region surrounding a supermassive black hole.
«We haven't, however, completely ruled out an association with the
magnetar or the other
stars of the cluster yet.
A giant flash
of energy from a supermagnetic neutron
star thousands
of light - years from Earth may shed a whole new light on scientists» understanding
of such mysterious
magnetars and
of gamma - ray bursts.
«The cluster
of stars also harbours a rare, extremely magnetic, neutron
star known as a
magnetar, but we think the gamma ray emission could be linked to the luminous blue variable
star.
If the young -
magnetar theory is correct, then — according to one possible version
of the story — we have to envisage a newborn, superdense neutron
star cloaked in a powerful and highly unstable magnetic field.
New data from these powerful telescopes later confirmed that 1E 1613 has the properties
of a
magnetar — a type
of neutron
star with an extremely powerful magnetic field — making it only the 30th known one.
Magnetars are a special kind
of neutron
star, and neutron
stars are a special kind
of dead
star.
They found it by observing a long - sought, short - lived afterglow
of subatomic particles ejected from a
magnetar — a neutron
star with a magnetic field billions
of times stronger than any on Earth and 100 times stronger than any other previously known in the Universe.