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The hydrogen line, 21 centimeter line, or H I line is a spectral line that is created by a change in the energy state of solitary, electrically neutral hydrogen atoms. It is produced by a spin-flip transition, which means the direction of the electron's spin is reversed relative to the spin of the proton. This is a quantum state change between the two…
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hydrogen line 21 cm 10 frequency energy arxiv radio bibcode doi s2cid neutral transition observed proton astro-ph state used wavelength
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| hydrogen clouds in our galaxy | instance of | It is commonly observed in astronomical settings | 0.80 | text |
| others.Because of the uncertainty principle | instance of | It is commonly observed in astronomical settings | 0.80 | text |
| its long lifetime gives an energy uncertainty on the order of 10 | instance of | It is commonly observed in astronomical settings | 0.80 | text |
| Hydrogen line | related to In radio astronomy | The | 0.60 | section |
| Hydrogen line | related to In radio astronomy | UHF | 0.60 | section |
| Hydrogen line | related to In radio astronomy | Electromagnetic | 0.60 | section |
| Hydrogen line | related to In radio astronomy | Earth's | 0.60 | section |
| Hydrogen line | related to In radio astronomy | Earth | 0.60 | section |
| Hydrogen line | related to In radio astronomy | Assuming | 0.60 | section |
| Hydrogen line | related to In radio astronomy | Doppler | 0.60 | section |
| Hydrogen line | related to In radio astronomy | Hence | 0.60 | section |
| Hydrogen line | related to In radio astronomy | It | 0.60 | section |
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