Since stars are born when dense
clouds of hydrogen molecules collapse, the rate of star formation and the availability of molecular hydrogen, the fuel for star formation, are inextricably linked.
Stars emerge when
clouds of hydrogen molecules coalesce under their collective gravitational attraction.
Not exact matches
Hydrogen molecules aren't the best coolant, but they are good enough to enable giant gas
clouds, millions
of times as massive as the sun, to fall in on themselves.
A molecular
cloud is an interstellar
cloud of dust, gas, and a variety
of molecules ranging from molecular
hydrogen (H2) to complex, carbon - containing organics.
Complex organic
molecules, consisting
of carbon bonded with other elements like oxygen and
hydrogen, are common in the Milky Way, but it was uncertain whether they would be produced in certain dwarf galaxies like the neighboring Large Magellanic
Cloud.
The researchers detected
molecules of carbon monoxide and two forms
of hydrogen in the
clouds, they report today in Astronomy & Astrophysics.
Detailed radio maps
of nearby molecular
clouds reveal that they are clumpy, with regions containing a wide range
of densities — from a few tens
of molecules (mostly
hydrogen) per cubic centimetre to more than one million.
Herzberg continued to add to his major scientific discoveries: he was the first to detect the
hydrogen molecule in planetary atmospheres, the first to uncover the presence
of water in comets, and the first to identify dozens
of free radicals (including methylene CH2 and methyl CH3) in the laboratory and interstellar
clouds.