「lines」の共起表現一覧(1語左が「emission」)
該当件数 : 24件
| dicates forbidden singly ionized iron emission | lines, Ca III] would be semiforbidden doubly ionized |
| exotic nature of its spectrum (bright emission | lines in lieu of dark absorption lines) it is also d |
| lem that for extended sources, nearby emission | lines will overlap. |
| The spectrum shows emission | lines of calcium in the H and K bands. |
| They found evidence for emission | lines of magnesium, silicon, sulphur, and various ot |
| It exhibits two sets of optical emission | lines with different redshifts. |
| Forbidden and semiforbidden emission | lines are enclosed by one or two brackets. |
| y optical spectra devoid of the broad emission | lines characteristic of quasars. |
| hat helium had been identified by the emission | lines in the Sun in 1868, and had then also been fou |
| M57 may include internal N II emission | lines located at the knots' tips that face the PNN; |
| se no known element was showing these emission | lines in the experiment it was concluded in the late |
| on, signifying that Pleione exhibits emission | lines in its spectrum rather than absorption lines, |
| meaning it shows prominent forbidden emission | lines of hydrogen in its spectrum. |
| So, it is possible that far-infrared emission | lines of •OH can be a good diagnostic of shock condi |
| Planetary nebula (PN) emission | lines were identified in this star in 1989 by the IU |
| aped sources shows the broad, optical emission | lines associated with quasar activity. |
| There, he studied emission | lines in the spectra of certain hot stars, and studi |
| Fluorescence gives rise to various emission | lines, the best-known of which is the iron feature a |
| The spectrum showed emission | lines of Fe XIII, which is heavily ionized iron that |
| disc, the spectrum of this star shows emission | lines and the magnitude varies over a period of abou |
| lain the appearance of absorption and emission | lines in stellar spectra. |
| t is difficult to detect far-infrared emission | lines from a quiescent molecular cloud. |
| large number of atomic absorption and emission | lines in the far-ultraviolet, FUSE enabled many stud |
| flame happens to contain a number of emission | lines which coincide with the vibrational frequencie |
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