The team used several hundred thousand compute hours at NERSC to produce a series of 2D and 3D simulations that helped them examine the role of dark matter halo photoevaporation — where energetic
radiation ionizes gas and causes it to disperse away from the halo — played not just in the early formation of stars but also the assembly of later galaxies.
Not exact matches
Producing artificial aurorae has taught scientists unexpected lessons about how
gases are
ionized in the ionosphere, a process that helps protect Earth from harmful ultraviolet solar
radiation.
As our solar system slowly orbits around the galactic center, the sun's ultraviolet
radiation carves out an egg - shaped region of
ionized hydrogen atoms surrounded by neutral hydrogen
gas.
One strong possibility is that the ultraviolet (UV)
radiation from the first - generation galaxies in the one - billion - year - old Universe
ionized the hydrogen
gas.
For most people, the risk of absorbing excess
ionizing radiation comes mainly through breathing radon, a
gas released by uranium and thorium in soils.
Measuring 300 light - years across, the bubble, known as G52L, is filled with hydrogen
gas that is
ionized by the energetic
radiation of embedded young stars.
«The UV
radiation from a massive star will
ionize and heat up disks of
gas surrounding nearby low - mass stars,» Bally says.
The intense
radiation from an AGN can
ionize the
gas around it (called photoionization), and this may be one mechanism at work in MAMMOTH - 1.
In follow - up observations from Kitt Peak National Observatory and the Lick Observatory, his team found 20 galaxies that had
gas that was
ionized by
radiation from a quasar, rather than from the energy of star formation.
In particular, one DOG (WISE1029 +0501, hereafter WISE1029) is outflowing
gas ionized by the strong
radiation from its supermassive black hole.
A widely accepted idea has described this phenomenon as: the strong
radiation from the galactic center in which the supermassive black hole locates
ionizes (* 1) the surrounding
gas and affects even molecular
gas that is the ingredient of star formation; the strong
radiation activates (* 2) or suppresses (* 3) the star formation of galaxies.
This discovery refutes existing theories, indicating that ultraviolet
radiation from the star would destroy molecular
gas and dust, and bringing the first direct detection of
ionized gas wind along with a supersonic jet and an accretion disk.
Stars emit UV
radiation and
ionizing photons necessary to heat and strip surrounding
gas.
Massive stars emit a large amount of ultraviolet
radiation that destroys the molecules and dust surrounding the star and creates
ionized gas, which in turn impedes the star's growth process.
«Photo - dissociation» or «Photon - dominated» Regions (PDRs) exist in the ISM at the interfaces between photo -
ionized and molecular
gas, where UV
radiation sets the ionization state, chemistry, and excitation at the edge of the molecular zone.
The warmer dust component is spatially correlated well with the [O III] emission and hence likely to be associated with the highly -
ionized gas locally heated by intense
radiation from the two clusters.