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Molecular cloud, also called dark nebula, interstellar clump or cloud that is opaque because of its internal dust grains.
A large molecular cloud also surrounds the SS 433/W50 system.
It was first detected in the Sagittarius B2 North molecular cloud (also known as the Sgr B2 Large Molecule Heimat source).
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The constellation also contains the conspicuous molecular cloud called the Coalsack.
Perseus also contains a giant molecular cloud, called the Perseus molecular cloud; it belongs to the Orion Spur and is known for its low rate of star formation compared to similar clouds.
Hydrogen cloud, also called H I region or H i region, interstellar matter in which hydrogen is mostly neutral, rather than ionized or molecular.
The gas is then part of a molecular cloud.
In this chain of events, the bright ultraviolet light from nearby stars heats the surface of the original molecular cloud.
He said that a dynamic front of stellar radiation "eats away" at the molecular cloud until it is stalled by a denser cloud core.
It is generally thought that brown dwarfs are formed, like stars, in the collapse of a heavy molecular cloud.
"When the ejecta hits the molecular cloud, the lumpy stuff in the clouds gets smashed into sheets that appear as long filaments," Dr. Chu said.
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