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Boxy isophotes, discs and dust lanes in elliptical galaxiesCCD images of 42 elliptical and S0 galaxies are examined for low-contrast structures or subtle distortions of the isophotes from perfect ellipses. 75 percent of the galaxies have isophotes completely describable as concentric ellipses to within the photometry errors. 'Boxy' isophotes, stellar discs, and dust lanes are detected in the remaining 25 percent of the sample. The boxy elliptical galaxies appear dynamically indistinguishable from normal ellipticals and are therefore different from boxy bulges, which rotate rapidly. Most of the galaxies with faint discs, however, appear dynamically similar to S0 galaxies. Nearly edge-on dust lanes are found in four galaxies, which suggests that dust lanes may commonly occur in elliptical galaxies.
Document ID
19860026173
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lauer, T. R.
(Lick Observatory, Santa Cruz, CA; Princeton University Observatory, NJ, United States)
Date Acquired
August 12, 2013
Publication Date
September 15, 1985
Publication Information
Publication: Royal Astronomical Society, Monthly Notices
Volume: 216
ISSN: 0035-8711
Subject Category
Astrophysics
Accession Number
86A10911
Funding Number(s)
CONTRACT_GRANT: NSF AST-81-20960
CONTRACT_GRANT: NSF AST-82-115511
CONTRACT_GRANT: NSG-7503
Distribution Limits
Public
Copyright
Other

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