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- W120734150 abstract "Attention is drawn to a group of stars of luminosity class Ia, in which variation of radial velocity has long been known in semi-regular cycles of 5 to 30 days. The interval of approximate repetition appears to be positively correlated with the luminosity of the star. Recent spectrophotometry of the absorption lines, especially by Rosendhal, Aydin, Groth, and Buscombe shows a considerable variation in the strength of Balmer lines (with emission components detected at H∝), as well as those of metallic ions. The microturbulence parameter derived from curves of growth for Fe ii varies by a factor of two or more during some cycles." @default.
- W120734150 created "2016-06-24" @default.
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- W120734150 date "1974-01-01" @default.
- W120734150 modified "2023-09-26" @default.
- W120734150 title "Variations in the Line Spectrum of A-Type Supergiants" @default.
- W120734150 doi "https://doi.org/10.1017/s0074180900237327" @default.
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