The Distribution of Disks in the μ0-log h Plane and the Inclination Correction

Details The Distribution of Disks in the μ0-log h Plane and the Inclination Correction The Distribution of Disks in the μ0-log h Plane and the Inclination Correction

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..275...21g&link_type=abstract

Disks of Galaxies: Kinematics, Dynamics and Peturbations, ASP Conference Proceedings, Vol. 275. Edited by E. Athanassoula, A. Bo

Astronomy and Astrophysics

Astronomy

Scientific paper

A further fundamental modification needs to be made to the Freeman
(1970) law, such that not only do LSB galaxies possess fainter central
surface brightnesses than the canonical Freeman value, but the upper
limit is in fact an upper (bright) `envelope' of points in the central
disk surface-brightness - log(scale-length) diagram, with slope ~2.

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