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| abstraction > mathematical concept > number > quantity > radiation measurement > spectral feature > spectral line > absorption line > interstellar line |
| interstellar line | ||||
| subject | fact | |||
| interstellar line | has width narrow | ![]() |
| has detection procedure narrow absorption lines which don't participate in the periodic Doppler shift of intrinsic absorption lines in a binary star | ![]() | |
| has equivalent width depends on the amount of absorbing matter between the source and the observer | ![]() | |
| has definition Sharp, distinct absorption lines superposed on stellar spectra, produced by the interstellar gas located between the source and the observer. Strongest are the D lines, followed by the H and K lines, and the K I doublet at 7699 and 7644 Å. | ![]() | |
| occurs in O stars | ![]() | |
| is a kind of absorption line | ![]() | |
| absorption line | has antonym emission line | ![]() |
| spectral line | has transition | ![]() |
| spectral feature | has wavelength | ![]() |
| has species | ![]() | |
| radiation measurement | has unit radiation unit | ![]() |
| number | has value | ![]() |
Kinds of interstellar line :