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U.S. Department of Energy
Office of Scientific and Technical Information

Program of ground-based astronomy to complement Einstein observations. Annual scientific report, 1 October 1983-30 September 1984

Technical Report ·
OSTI ID:5660373
The objective of the funded research is the formulation and execution of ground-based astronomical observations and interpretive studies complementary to the x-ray data accumulated with the Einstein satellite, to be used in addressing a number of questions of current astrophysical interest. During the past year, the program focussed on two main topics: the processes leading to high-energy emission in the winds and coronae of late-type stars, and the structure and evolution of supernova remnants and the neutron stars they may contain. The stellar work encompasses the development of a complete, x-ray flux-limited sample of stars which, when combined with a complete, magnitude-limited optical sample will provide the best available description of the distribution of coronal activity in stars of spectral types F through M. A principal corollary of this work is the determination of the contribution of coronally active M dwarfs to the diffuse x-ray background. Star-cluster studies are combined with the survey work toward the goal of specifying the critical factors governing the production and evolution of magnetically dominated coronae in late-type stars. The supernova remnant work concentrates on the twin problems of the evidence for and frequency of neutron-star formation in supernova explosions and the time development of the luminosity and size of the expanding supernova shock wave.
Research Organization:
Columbia Univ., New York (USA). Columbia Astrophysics Lab.
OSTI ID:
5660373
Report Number(s):
AD-A-151111/2/XAB; CAL-1553
Country of Publication:
United States
Language:
English