The dark dust filaments that lace M20 were created in the atmospheres of
cool giant stars and in the debris from supernovae explosions.
Not exact matches
The form of Real Madrid goalkeeper Iker Casillas could mean the Spanish
giants decide to
cool their pursuit of Manchester United
star David de Gea.
In short order, astronomically speaking, the red
giant blows off its outer layers and leaves behind a white dwarf — essentially the naked heart of the
star — which slowly
cools to eternal blackness.
This gal thinks scientists are
cooler than rock
stars: Shirley Ann Jackson, recites Lia in an excited crescendo, «explores the invisible particles that make up everything in the universe, including you and me and your computer and Limburger cheese and the rings of Saturn and even
giant squids!»
Their temperatures can range from nearly as hot as a
star to as
cool as a planet, and their masses also range between
star - like and
giant planet - like.
Take Mira, a relatively
cool, older
star known as a red
giant, which lies 350 light - years away in the constellation Cetus.
You're seeing
cooler red
stars and red
giants, and you're certainly able to see things that you couldn't see on a visible spectrum [source: IPAC].
These early images, which show
giant planets in
cool orbits far from the glow of their
stars, represent a huge technological leap.
However, we find a significant variation of the fraction of
cool dwarfs with galactic latitude, indicating a target selection bias due to interstellar reddening and the increased contamination by
giant stars near the galactic plane.
According to Professor Jim Kaler at the University of Illinois» Department of Astronomy, Rana started life as a main sequence F8 dwarf (somewhat hotter and brighter than Sol with slightly greater mass) around 7.5 billion years ago, but core hydrogen fusion has ceased causing the
star to expand and
cool as an active subgiant before becoming much brighter and larger «as a true
giant star» through core helium fusion.
According to astronomer Catherine Pilachowski (who wrote an analysis of HE 0107 - 5240's discovery for Nature), HE 0107 - 5240 contains a «striking excess» of nitrogen and carbon although these elements not usually abundant in
stars of the
cool,
giant family to which the
star belongs.
Gacrux is a
cool red
giant star of spectral and luminosity type M3.5 III (but was once thought to be a «bright
giant» of luminosity type II).
This material gathers into huge turbulent reservoirs of
cool, low - density gas, extending more than 30 000 light - years from the galaxy's
star forming region [3] These turbulent reservoirs of diffuse gas may be of the same nature as the
giant glowing haloes seen around distant quasars..
Information about the ang... ▽ More When the core hydrogen is exhausted during stellar evolution, the central region of a
star contracts and the outer envelope expands and
cools, giving rise to a red
giant, in which convection occupies a large fraction of the
star.
These extended,
cool and hence red
stars are key targets for stellar evolution studies as well as galactic studies for several reasons: a) many
stars go through a red -
giant phase; b) red
giants are intrinsically bright; c) large stellar internal structure changes as well as changes in surface chemical abundances take place over relatively short time; d) red -
giant stars exhibit global intrinsic oscillations.
Abstract: When the core hydrogen is exhausted during stellar evolution, the central region of a
star contracts and the outer envelope expands and
cools, giving rise to a red
giant, in which convection occupies a large fraction of the
star.
As a highly evolved and relatively
cool orange - red
giant, single
star, Pollux is not much like its «twin»
star Castor, which is actually composed of three sets of binary
stars (as many as four bluish - white, main sequence
stars with two fainter companions).