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abstraction > mathematical concept > number > quantity > radiation measurement > spectral feature > spectral line > absorption line > interstellar line |
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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 :