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    the SB profile of a typical dE galaxy in the Virgo cluster This profile is nearly straight because it fits the exponential law well The violet curve shows the SB profile of another galaxy which is thought to be a

    Original URL path: http://www.astro.queensu.ca/~courteau/Phys216/images/pics/ede.html (2016-02-13)
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    218 333 King model brightness profiles The scale is one for which the de Vancouleurs law is a straight line Curves having 2 c 2 35 are generally the best

    Original URL path: http://www.astro.queensu.ca/~courteau/Phys216/images/pics/kingmod.html (2016-02-13)
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    μ sky 22 mag sq arcsec O Neil Bothun and Correll 1997 AJ 113 1212

    Original URL path: http://www.astro.queensu.ca/~courteau/Phys216/images/pics/sbprof.html (2016-02-13)
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    Carignan and Purton 1998 ApJ 506 125

    Original URL path: http://www.astro.queensu.ca/~courteau/Phys216/images/pics/h1map.html (2016-02-13)
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    Rubin et al 1985 ApJ 289 81 More luminous galaxy means higher V rot Tully Fisher Relation log R 25 0 249 M B 4 00 R 25 in kpc

    Original URL path: http://www.astro.queensu.ca/~courteau/Phys216/images/pics/htype.html (2016-02-13)
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    Rubin et al ApJ 289 81

    Original URL path: http://www.astro.queensu.ca/~courteau/Phys216/images/pics/tf.html (2016-02-13)
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    that of Fig 2 and eq 2 although it shows 10 larger scatter primarily due to larger observational uncertainties Note choice of axes to see FP Pahre et al 1998 AJ 116 1591 Kormendy relation between effective radius and mean surface brightness The best fitting relation is R eff Σ K eff 0 61 0 07 with a scatter of 0 227 dex in log R eff which is 2

    Original URL path: http://www.astro.queensu.ca/~courteau/Phys216/images/pics/fj.html (2016-02-13)
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    Carollo et al 1995 ApJ 441 25 Note rotation of some of these E galaxies

    Original URL path: http://www.astro.queensu.ca/~courteau/Phys216/images/pics/los.html (2016-02-13)
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