| 41. | O ), and ) give rise to the 500.7 nm emission line and others.
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| 42. | The emission line spectrum associated with dense stellar winds has persisted ever since the late 19th century.
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| 43. | Its characteristic emission lines are produced by gas moving at high speeds around the central black hole.
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| 44. | Have you noticed on that applet that the absorption lines are the same as the emission lines.
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| 45. | SN 2002cx was by then in the nebular phase, with emission lines dominating over absorption lines.
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| 46. | Emission lines of this star are those of the disk of material, not the star itself.
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| 47. | The strongest hydrogen emission line at 656.3 nm gives H II regions their characteristic red colour.
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| 48. | They may also display very complex H? profiles, typically having strong emission lines combined with absorption lines.
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| 49. | The SIGMA telescope aboard GRANAT detected a relatively narrow variable emission line near 500 keV in the spectrum.
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| 50. | The divergences with the straight line are due to the absorptions and emission lines in the stellar spectra.
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