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Titlebook: Astronomy and Astrophysics Abstracts; Literature 1982, Par S. Böhme,W. Fricke,G. Zech Book 1982 Springer-Verlag Berlin Heidelberg 1982 astr

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D. Deepak,S. Srivastava,N. K. Khare,A. Khare .C(., .).O reaction serving as the energy and neutron production source. Thermal runaway leads to a slowly rising neutron flux which causes a buildup of heavier elements from lighter ones; in the final stages of the thermal flash the nuclei are transformed into an .-process distribution. It is of p
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https://doi.org/10.1007/978-3-7091-6578-2ive to photospheric parameters. A secular decrease of equivalent widths ranging from 0 to 2.3% is observed. The authors conclude that the line weakenings are due to global variations of surface properties. Model atmosphere analysis suggests that the observed response pattern reflects a slight flatte
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https://doi.org/10.1007/978-3-7091-8906-1alogs. Fifty-two of the stars had no previously published velocities. Spectral types have been assigned, and space motions are computed using the newly determined radial velocities and previously published parallaxes and proper motions. Several high velocity stars are found, but one particularly int
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https://doi.org/10.1007/978-3-7091-8551-3the presence of an interesting correlation between the gas and dust in this region. A dust filament is shown to run parallel to, but displaced towards the galactic plane from, a ridge of enhanced H I emission. It is suggested that this results from the passage of a shock wave through the system, res
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https://doi.org/10.1007/978-3-7091-9084-5Astronomy and Astrophysics Abstracts begins documentation and abstracting from the year 1969. For information on astronomical literature before this date consultation of one of the following bibliographies is suggested:
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Naturally Occurring Perylenequinones,The foundation is described for understanding the chemical composition of the inner core, the core and the lower mantle of the Earth.
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