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- W3121743325 endingPage "92" @default.
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- W3121743325 abstract "According to one version of the recently proposed manifold theory that explains the origin of spirals and rings in relation to chaotic orbits, galaxies with stronger bars should have a higher spiral arms pitch angle when compared to galaxies with weaker bars. A sub-sample of barred-spiral galaxies in the Ohio State University Bright Galaxy Survey, was used to analyze the spiral arms pitch angle. These were compared with bar strengths taken from the literature. It was found that the galaxies in which the spiral arms maintain a logarithmic shape for more than 70$degr$ seem to corroborate the predicted trend." @default.
- W3121743325 created "2021-02-01" @default.
- W3121743325 creator A5080982762 @default.
- W3121743325 date "2011-12-19" @default.
- W3121743325 modified "2023-10-16" @default.
- W3121743325 title "TESTING THEORIES IN BARRED-SPIRAL GALAXIES" @default.
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- W3121743325 doi "https://doi.org/10.1088/0004-637x/744/2/92" @default.
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