Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 15 January 1993:
Vol. 259. no. 5093, pp. 327 - 334
DOI: 10.1126/science.259.5093.327

Articles

Far-Ultraviolet Astronomy on the Astro-1 Space Shuttle Mission

Arthur F. Davidsen 1

1 Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218

The Astro-1 mission obtained observations related to a wide variety of current problems in astronomy during a 9-day flight of the space shuttle Columbia. Early results from one of the instruments, the Hopkins Ultraviolet Telescope, are reviewed here. Among these are new insights concerning the origin of the ultraviolet light from the old stellar population in elliptical galaxies, new evidence for a hot, gaseous corona surrounding the Milky Way, improved views of the physical conditions in active galactic nuclei, and a measurement of the ionization state of the local interstellar medium.


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Radio Emission from the Heliopause Triggered by an Interplanetary Shock.
D. A. Gurnett, W. S. Kurth, S. C. Allendorf, and R. L. Poynter (1993)
Science 262, 199-203
   Abstract »    PDF »



To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)