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- W2034982920 abstract "Recently it has been suggested that spiral galaxies are opaque in the B band [Valentijn, Nature, 346, 153 (1990)]. We have investigated the dependence of surface brightness on inclination for galaxies in the near-infrared H band, where absorption by dust affects the light to a much lesser extent. By examining large samples with data from the literature, together with some new surface photometry, we find that spirals behave in a semi-transparent way, with face-on absorption in H averaging ≃0.10 mag. From near-infrared images we find that the scale height of the dust in spiral galaxies is ≃0.5-0.6 times that of the stars" @default.
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- W2034982920 date "1992-06-01" @default.
- W2034982920 modified "2023-09-25" @default.
- W2034982920 title "How transparent are spiral galaxies in the near infrared?" @default.
- W2034982920 doi "https://doi.org/10.1086/116193" @default.
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