The orientation of spin vectors of galaxies in the Ursa Major filament

Abstract

view Abstract Citations (20) References (22) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Orientation of Spin Vectors of Galaxies in the Ursa Major Filament Han, Cheongho ; Gould, Andrew ; Sackett, Penny D. Abstract Spin vectors of 60 galaxies in the "Ursa Major filament" are obtained from CCD images and spectroscopic determinations of the directions of rotation. These data are used to remove the fourfold degeneracy introduced by the projected images of galaxies, making possible the complete reconstruction of the galaxy spin vectors. Several possible organizations of spin vectors are investigated by means of statistical analyses of the three-dimensional spin vector maps. The results indicate that there exists no significant alignment of galaxy spin vectors with respect to the supergalactic plane, the supergalactic axis, or the cylindrical axis of the filament itself. No tendency for linear alignment of spin vectors toward any specific direction was detected. We also obtain a statistically negative result for azimuthal, radial, and circular-helical orientation of spin vectors. Publication: The Astrophysical Journal Pub Date: May 1995 DOI: 10.1086/175671 arXiv: arXiv:astro-ph/9408022 Bibcode: 1995ApJ...445...46H Keywords: Alignment; Attitude (Inclination); Galactic Rotation; Galaxies; Sky Surveys (Astronomy); Spin Dynamics; Charge Coupled Devices; Data Correlation; Radial Velocity; Red Shift; Spectrum Analysis; Statistical Analysis; Astronomy; GALAXIES: FUNDAMENTAL PARAMETERS; GALAXIES: KINEMATICS AND DYNAMICS; Astrophysics E-Print: 20 pages, 4 figures, request PostScript file to cheongho@payne.mps.ohio-state.edu, OSU-TA-14/94 full text sources arXiv | ADS | data products SIMBAD (99) NED (94)