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- W1976158121 abstract "IN recent years evidence has been brought forward by several investigators1 indicating that light from distant stars suffers a slight attenuation in travelling through interstellar space. In particular a recent investigation by Jones2 assigns fairly definite numerical values to coefficients of attenuation corresponding to “photographic” and “visual” light from stars of known proper motions and spectral types the magnitudes of which had been carefully measured by Parkhurst3 for light of these wave-lengths. If, as seems reasonable, this extinction is assumed to be due to attenuation by scattering in travelling through a “residual” gas occupying, interstellar space, we are enabled to estimate the average density of molecules in the intervening regions, following a method due originally to Larmor4 for assigning an upper limit to the density of matter in comets' tails." @default.
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- W1976158121 date "1915-08-01" @default.
- W1976158121 modified "2023-09-30" @default.
- W1976158121 title "The Density of Molecules in Interstellar Space" @default.
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- W1976158121 doi "https://doi.org/10.1038/095701b0" @default.
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