Fig 1 - uploaded by Nilkanth Vagshette
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(B-R) color maps derived for the target galaxies after comparing the light distribution in two different pass band images B and R. In first row, NGC 1482 (top left), NGC 2685 (middle) & NGC 3955 (top right) where as second row: NGC 5354 (bottom left) & NGC 5866 (bottom right)
Source publication
We present multiwavelength analysis of a heterogeneous sample of early-type galaxies
selected from different environments i.e. fields, groups and clusters. Optical imaging
analysis of these galaxies reveals variety of morphological form of dust i.e., lanes,
filaments, clumps, etc. with their extinction properties identical to those seen in our
own...
Contexts in source publication
Context 1
... analysis has enabled us to derive morphology of dust in the target galaxies. The dust occupied region are shown in color maps derived for the target galaxies in R-band subtracted from B-band are shown in Figure 1, where brighter shades represent regions associated with the dust extinction. In order to investigate the dust extinction properties in target galaxies we have generated their extinction maps. ...
Context 2
... analysis has enabled us to derive morphology of dust in the target galaxies. The dust occupied region are shown in color maps derived for the target galaxies in R-band subtracted from B-band are shown in Figure 1, where brighter shades represent regions associated with the dust extinction. In order to investigate the dust extinction properties in target galaxies we have generated their extinction maps. ...
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