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The University of Toledo Ritter Astrophysical Research Center Toledo, Ohio 43606 This report covers the period 1 July 1999 to 30 June 2000. 1 Personnel 3 3.1 Research Stellar Astrophysics During the

Bjork. The University retained the contract astrophysics and astronomy contract of the former NASA Astrophysics Division, headed by D. Kornberg as a single center, whose activities in the field of stellar astrophysics are reported in this report. Kornberg has made major contributions to the field of stellar astronomy since his appointment. He has published three important reviews: The New York Times, Science, Science, and Astrophysics, as well as A New Understanding of Black Holes, submitted to American Physicist and Astronomy, and in the American Journal of Physics. The reviews have been widely accepted throughout America and Europe. 1.2 Research Near-Earth Object Surveying In the summer of 1995, an steroidal sample arrived in Earth's orbit, carrying samples from a variety of celestial bodies (Buchanan et al., 1996). The object's trajectory and orbital characteristics are a unique opportunity to investigate the behavior of interstellar material. 2. Results Data from this research project were available to the staff in November 1995, and they were analyzed and reported by W. Kornberg during the course of the year. 3.1 Data Acquisition The research project involved the acquisition, with the help of the university's telescope/astronomy facilities, of more than 3000 high-quality images from the Hubble camera. The data were processed by the Stellar Astrophysics Research Group in a series of “color” images, in which each color band has eight adjacent values in the visible spectrum at different depths. The color bands are a product of a spectral decomposition of the data. Three color bands are defined to denote different levels of stellar spectral energy distribution. The three bands differ in their relative intensity in this order: red; green; blue. The first band (“red band” or “red band 2”) represents a spectral peak at 9082 nm, the second (“green band” or “green band 8”) represents a peak at 9076 nm, and the third (“blue band” or “blue band 3”) represents a spectral peak at 9107 nm. The data were organized into 20-bit channels, where the width of the channel equals one-eighth of the spectral depth. The order of the channels in a channel was determined during image analysis via a series of mathematical procedures based on the “red band” in the red image. The order was chosen in such a way that each order has a common value for each part of the spectrum.

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