
This contribution attempts to reconstruct the precise history of the discovery of one of astronomy's long-lasting enigmas, the so-called diffuse interstellar bands (DIBs). While systematic research into the DIBs was initiated by Merrill in 1936, the first pointers to abnormal features in the spectra of distant stars were published some 15 years earlier by Mary Lea Heger, who researched them at Lick Observatory while a student. We have examined Heger's observing notebooks from her doctoral work in 1919–1920. We have also digitized her 1919 photographic plates, and compared the spectra that she measured with modern ones. Our conclusion is that Heger was indeed the first to observe and draw attention to the two absorption features at 5780 Å and 5797 Å that subsequently came to be recognized as DIBs, thereby initiating a substantial field of research that now embraces several hundred such features, all of whose provenance is unsolved even to this day.
Diffuse interstellar bands, History, Lick observatory, Systematic research, Research, Astronomy, Long lasting, Observatories, Mary Lea Heger, Buildings
Diffuse interstellar bands, History, Lick observatory, Systematic research, Research, Astronomy, Long lasting, Observatories, Mary Lea Heger, Buildings
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 45 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 10% | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 10% |
