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are differentiated by the character of the ab-
                                         sorbent vapours of their atmospheres.
                                            It is very likely that, after the chemists
                                         have taught us how to interpret all the va-
                                         rieties of spectrum, it will be possible to as-
                                         cribe the different spectrum-classes to dif-
                                         ferent stages in the life-history of every star.
                                         Already there are plenty of people ready to
                                         lay down arbitrary assumptions about the
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