Examples of using Interstellar clouds in English and their translations into Spanish
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These interstellar clouds are immense.
Deep in space there are giant interstellar clouds.
In interstellar clouds, cosmic rays leave behind a trail of H+ 2, and therefore H+ 3.
The most abundant molecule in dense interstellar clouds is H2.
Interstellar clouds like the Orion Nebula are found throughout galaxies such as the Milky Way.
Stars are born in litters,formed from the gas and dust of interstellar clouds.
The average density of HI interstellar clouds is in the range 0.1-1000 atoms per cubic cm.
Its third objective is to detect the stars of our galaxy obscured by interstellar clouds.
In interstellar clouds, there was proto stellar disks from which escapes a bipolar ejection of material.
H+ 3 has been detected in two types of celestial environments:Jovian planets and interstellar clouds.
Eventually, their stars will carry them through other interstellar clouds, where they may seed still more new worlds.
Several interstellar clouds have been observed and the presence of the condensation of very cold interstellar matter unknown so far has been revealed.
The dominant destruction pathway in dense interstellar clouds is by proton transfer with a neutral collision partner.
M34 lies in the plane of our Galaxy,it will eventually be dispersed under the effects of tidally related to encounters with interstellar clouds of the Milky Way and other stars.
Theoretical modelling of ice formation in interstellar clouds suggests that comet Hale-Bopp formed at temperatures of around 25-45 kelvins.
During each revolution around the galaxy,our solar system will pass through two or three gigantic interstellar clouds, each of them many light years across.
Most standard(baryonic) matter is found in intergalactic gas,stars, and interstellar clouds, in the form of atoms or ions(plasma), although it can be found in degenerate forms in extreme astrophysical settings, such as the high densities inside white dwarfs and neutron stars.
The new very sensitive instruments of the telescope will allow to drill the space which is darkened by clouds of gas, the interstellar clouds which block telescopes working in the visible domain.
HeH+ could be formed in the cooling gas behind dissociative shocks in dense interstellar clouds, such as the shocks caused by stellar winds, supernovae and outflowing material from young stars.
The ratio of deuterium to normal hydrogen was found to vary from compound to compound,which astronomers believe suggests that cometary ices were formed in interstellar clouds, rather than in the solar nebula.
Absorption spectroscopy has been particularly important for understanding interstellar clouds and determining that some of them contain molecules.
A nebula is an interstellar cloud of gust and gas. Hydrogen.
Its sister stars,hatched from the same interstellar cloud, are dispersed throughout the galaxy.
The nebula is a giant interstellar cloud, 100 light-years across, where stars are forming.
The Lagoon Nebula is a giant interstellar cloud attractive and fascinating located about 4 to 5 thousand light years away in the constellation Sagittarius the Archer.
When our solar system passes through an interstellar cloud, the gravity of the massive cloud stirs up the outermost comets.
A dark nebula is a type of interstellar cloud so dense that it obscures the light from background stars.
After thousands of years,fragments of the rocks ejected from Earth can fall as meteors into the atmospheres of newborn planets in the interstellar cloud.
One of Jeans' major discoveries, named Jeans length,is a critical radius of an interstellar cloud in space.
The North America Nebula and the nearby Pelican Nebula(IC 5070)are parts of the same interstellar cloud of ionized hydrogen H II region.