The galaxy formed 11 billion years ago, and its star - forming gas has one of
the highest ionized gas velocity dispersions ever measured.
Not exact matches
When a particle hits a hard surface at
high speeds, it vaporizes and
ionizes the target, releasing a cloud of dust,
gas and plasma.
The hiss occurs throughout the plasmasphere (the zone thousands of miles above the earth that teems with
ionized gases), removing the plasmasphere's
high - energy electrons and tempering their lethal power.
A team led by scientists from the University of California, Los Angeles and the Department of Energy's SLAC National Accelerator Laboratory has reached another milestone in developing a promising technology for accelerating particles to
high energies in short distances: They created a tiny tube of hot,
ionized gas, or plasma, in which the particles remain tightly focused as they fly through it.
A
high voltage on the electrodes
ionizes the
gas, converting it into a plasma.
The amount of
ionizing energy inputted into the
gas by newly formed stars is much
higher in the early universe.
However, this sealing process requires exposure of the device components to
high energy or «
ionized»
gas and whether biomolecules can survive this harsh process is unknown.
As a plasma, helium's electrons and protons are not bound together, resulting in very
high electrical conductivity, even when the
gas is only partially
ionized.
«Probing the Conditions at
Ionized / Molecular
Gas Interfaces With
High Resolution Near - Infrared Spectroscopy»
Shao and collaborators now combine the previous Cycle 0 ALMA observations of ULAS J1319 +0950 with new,
high - resolution observations from Cycle 1 to draw a detailed picture of where the dust and the atomic and
ionized gas (which traces the star formation) reside in this galaxy's core.
Here the cycle is
ionize the
gas to make the plasma, build up the current, heat the plasma with an external heater until the temperature for fusion is reached, turn off the heater, and then have the energy require to keep the temperature
high generated by the fusion reaction itself.
«The solar wind, because it is an extended
ionized gas of very
high electrical conductivity, drags some magnetic flux out of the Sun, thereby filling the heliosphere with the weak interplanetary magnetic field.