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A molecular cloud—sometimes called a stellar nursery if star formation is occurring within—is a type of interstellar cloud of which the density and size permit absorption nebulae, the formation of molecules (most commonly molecular hydrogen, H2), and the formation of H II regions. This is in contrast to other areas of the interstellar medium that contain…
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molecular cloud gas clouds stars interstellar hydrogen formation dust astronomers star density radio cores regions co molecules clumps 10 h2
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| methanol | instance of | Astronomers have observed the presence of long chain compounds | 0.80 | text |
| ethanol | instance of | Astronomers have observed the presence of long chain compounds | 0.80 | text |
| benzene rings | instance of | Astronomers have observed the presence of long chain compounds | 0.80 | text |
| their several hydrides | instance of | Astronomers have observed the presence of long chain compounds | 0.80 | text |
| Molecular cloud | related to Cloud formation and destruction | Due | 0.60 | section |
| Molecular cloud | related to Cloud formation and destruction | By | 0.60 | section |
| Molecular cloud | related to Cloud formation and destruction | The | 0.60 | section |
| Molecular cloud | related to Cloud formation and destruction | Only | 0.60 | section |
| Molecular cloud | related to Cloud formation and destruction | Milky Way | 0.60 | section |
| Molecular cloud | related to Cloud formation and destruction | Two | 0.60 | section |
| Molecular cloud | related to Cloud formation and destruction | Cloud | 0.60 | section |
| Molecular cloud | related to Cloud formation and destruction | Models | 0.60 | section |
These clusters group vocabulary that occurs around closely connected concepts in the source material.
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