No CrossRef data available.
Article contents
Schmidt-Plate Astrometry – Dinosaurs in Action
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Photographic plates are well established as stable detectors, well suited for positional astronomy. The completion of the current second epoch 48 inch Schmidt surveys in both hemispheres will provide material spanning baselines of 20–45 years, allowing proper motions to be determined to an accuracy of 4–7 mas yr−1. This paper discusses some of the Galactic structure problems that these data, combined with accurate photometry, can be used to address.
- Type
- VIII. Schmidt Astrometry
- Information
- International Astronomical Union Colloquium , Volume 148: The Future Utilisation of Schmidt Telescopes , 1995 , pp. 208 - 217
- Copyright
- Copyright © Astronomical Society of the Pacific 1995
References
Evans, D.W., 1993, In Galactic and Solar System Optical Astrometry, Morrison, L.V. & Gilmore, G.F., edsGoogle Scholar
Luyten, W.L., 1974, Proper Motion Survey with Forty-Eight Inch Telescope, XXXVIII, (Univ. of Minnesota, Minneapolis)Google Scholar
Majewski, S.R., 1994, In Astronomy from Wide-Field Imaging, Proc. IAU Symp. 161, (Kluwer, Dordrecht), in pressGoogle Scholar
Monet, D.G., 1994, In Astronomy from Wide-Field Imaging, Proc. IAU Symp. 161, (Kluwer, Dordrecht), in pressGoogle Scholar
Monet, D.G., Dahn, C.C., Vrba, F.J., Harris, H.C., Pier, J.R., Luginbuhl, C.B. & Ables, H.D., 1992, AJ, 103, 638
Google Scholar
Scholz, R.D., 1994, in Astronomy from Wide-Field Imaging, Proc. IAU Symp. 161, (Kluwer, Dordrecht), in pressGoogle Scholar
You have
Access