Abstract
Surface brightness distributions in the faint outer regions of 19 elliptical and S0 galaxies are presented, and it is argued that these distributions are more reliable than those previously published. Systematic errors in low surface brightness photometry are discussed. The forms of the surface brightness profiles are compared with the isophote shapes of the galaxies, and a number of interesting correlations emerge, although the sample of galaxies is too small to draw any firm conclusions.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
