... in a single central 4в4 sq deg field (paper I, Davies et al., 2010), how the cluster environment truncates the dust discs of spiralgalaxies (paper II, Cortese et al., 2010), the dust life-time in early-type galaxies (paper III, Clemens et al., 2010), the ...
... environment truncates the dust discs of spiralgalaxies (Cortese et al. 2010b, Paper ... 2010, Paper III), the spiralgalaxy dust surface density and MNRAS 438, 19221947 ...
... A barred spiral with marked similarities to our home Milky Way Galaxy , NGC 1808 is distinguished by a peculiar nucleus , an unusually warped disk , and strange flows of hydrogen gas out from the central regions. ...
... typ e galaxy (HRS48, middle row) and un-detected elliptical and its spiral companion ... which focused on Hi-normal spiralgalaxies only, this analysis takes advantage of a ...
... JPEG (116 k) , Tiff (2.8 M) , PS (5.9 MB) NGC 3603 is a bustling region of star birth in the Carina spiral arm of the Milky Way galaxy, about 20,000 light-years from Earth. ...
... Many authors proposed a lot of different solutions: circumnuclear star clusters, bars, disks or nuclear spirals, interactions between galaxies, and mergers. ...
... the cool 20 K dust OS SLUGS results: submm morphology Detected 52 galaxies in the OS sample, 17 of which also detected at 450m Several common features in the submm morphology of spirals: many exhibit two peaks of 850-m emission, seemingly coincident ...