This animation shows how the exoplanet KELT - 9b is losing part of its substance due to
intense radiation from its star.
This nebula glows because of
the intense radiation from the star Xi Persei.
Not exact matches
Emission nebulae like IC 2944 are composed mostly of hydrogen gas that glows in a distinctive shade of red, due to the
intense radiation from the many brilliant newborn
stars.
The massive black hole shown at left in this drawing is able to rapidly grow as
intense radiation from a galaxy nearby shuts down
star - formation in its host galaxy.
Intense radiation from the brilliant central
stars is causing hydrogen in the nebulae to glow pink.
A nearby
star features a comet - like tail that could be the outer reaches of a protoplanetary disk evaporating under the
intense ultraviolet
radiation from IRS 2.
According to new observations
from NASAs Hubble Space Telescope of a
star - forming region in a nearby galaxy known as the Large Magellanic Cloud,
intense radiation and powerful winds
from massive, ultrabright baby
stars have sculpted their environment, carving a large cavity in their natal nebula, N83B.
Extremely turbulent environments can disrupt the normal procession of material onto a protostar, while
intense radiation —
from massive nearby
stars and supermassive black holes — can blast away the parent cloud, thwarting the formation of all but the most massive of
stars.
The
intense radiation and strong outflows
from these massive
stars caused nearby gas to dissipate.
This is because «cooked planets,» or those that lie close to their host
stars, are stripped off of their atmospheres due to
intense radiation coming
from the fiery, heavenly bodies.
The first
stars, however, also began emitting
intense ultraviolet
radiation that «re-ionized» neutral hydrogen atoms formed after the Big Bang by tearing electrons
from their proton nuclei.
Many
stars are forming inside these huge columns which are being blasted by
intense radiation from many of the nearby
stars.
The donut of material confines the
intense radiation coming
from the remnant of the dying
star.