Are Spiral Disks Really Opaque ?

dc.creatorXu, C.
dc.creatorBuat, V.
dc.date1994-11-24
dc.date.accessioned2026-07-07T02:19:36Z
dc.date.available2026-07-07T02:19:36Z
dc.descriptionWe compare the ultra-violet, optical, and far-infrared emission for a sample of 135 spiral galaxies in order to address the widely debated problem concerning the opacity of spiral disks. We find that the re-radiation of the dust, estimated from the far-infrared emission, is on average only 31$\pm 1$ percent of the bolometric luminosity of a spiral galaxy, indicating that less than one third of the stellar radiation is absorbed and then re-radiated by dust in a spiral disk. Applying a radiation transfer model which assumes a `Sandwich' configuration for the spiral disk, and fully takes into account the effect of scattering, we find for our sample a median of the face-on blue (4400Å) optical depth $\rm τ_B=0.49$ and the mean $\rm <τ_B> =0.60\pm 0.04$, indicating that most spiral galaxies in our sample are {\it not} opaque for blue light ($\rm τ_B <1$).
dc.description4 pages of uuencoded postscript file, accepted as a Letter to Astronomy and Astrophysics. 3 of 4 figures (Figures 1, 2, 4) are in a separate file. Figure 3 is available on request
dc.identifierhttps://arxiv.org/abs/astro-ph/9411101
dc.identifierhttp://arxiv.org/abs/astro-ph/9411101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9926
dc.subjectAstrophysics
dc.titleAre Spiral Disks Really Opaque ?
dc.typetext

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