... nature of starburst dust, we constructed a model of the stars and dust in starburst ... dust were computed for average Milky Way (MW) and Small Magellanic Cloud (SMC) dust ...
... dust continuum observations of the edge-on spiral galaxy NGC 4565 in all Herschel ... dust energy budget of NGC 4565 suggests that a sizable fraction (two-thirds) of the ...
... dust-scattering, -absorbing, and -emitting properties are calculated from realistic ... The dust temperature and the emitted dust spectrum are calculated self-consistently ...
... the link between dust and attenuation is not straightforward and depends on both the amount of dust and its distribution ... with the dust, suggesting that the distribution of stellar reddening acts as a poor tracer of the overall dust content ...
... dust that accompanies star formation in the local Universe, where the dust-to-gas ... dust emission from IZw18, from which we determine its dust mass to be 450-1,800 ...
... dust model (amorphous silicate and carbonaceous grains), for each pixel in each galaxy we estimate (1) dust mass surface density, (2) dust mass fraction contributed by polycyclic aromatic hydrocarbons, (3) distribution of starlight intensities heating the ...
... dust and the effective temperatures or bolometric magnitudes of stars in the H II regions, suggesting that the H II region ... as a trend in the temperature of a minority hot dust component, while a majority of the dust remains significantly cooler ...
... Enhanced dust heating in the bulges of early-type spiral galaxies . ... affect the temperatures of the cool (T ~ 20-30 K) dust component in the inner regions of galaxies, which implies that the ratio ...