Correlation among Morphological Classifications and Mass to Luminosity(m/l) Ratios of Extra Galaxies

Astronomy and Astrophysics – Astronomy

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Scientific paper

Morphological luminosity parameters(¥ìe, re, ¥ìo, ¥á-1) and D/B were estimated from the decomposition of surface brightness distributions of 28 extra galaxies. Decomposition was made using the standard non-linear least square fitting method and we used the seeing convolved model to get the central brightness of these galaxies. Masses and M/LB were calculated using rotational velocities of these galaxies from the fitting to the generalized Toomre's mass model.

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