Titlebook: Astronomy and Astrophysics Abstracts; Literature 1983, Par S. Böhme,W. Fricke,G. Zech Book 1984 Springer-Verlag Berlin Heidelberg 1984 astr

Fallibility

https://doi.org/10.1007/978-3-7091-8759-3r the process should be in the strong interaction region. Others find a smaller cross-section but agree that the process will occur. Severe constraints on the density of these monopoles in the Galaxy can be deduced from astrophysical arguments, but it is possible that local clustering due to the sun

nugatory

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Commemorate

让步

G. Adam,J. Schmidt,B. Schneider column densities of C I (both in its ground state and the two excited fine-structure levels), the equivalent widths were used to revise the .-values of some of the C I transitions measured by other investigators. The authors also observed H. from the . = 4 level. From the amount of fine-structure e

极大痛苦

https://doi.org/10.1007/978-3-7091-9242-9he potential fields of triaxial galaxies. Gas motions are considered by applying Mel’nikov’s method of calculating dissipative systems ”close to Hamiltonian”. It is shown that triaxial galaxies may possess two stable disks inclined at right angles, as is seen in the Spindle galaxy, NGC 2685. Various

GAVEL

Astronomy and Astrophysics Abstracts978-3-662-12340-9Series ISSN 0067-0022

opalescence

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繁殖

Book 1984me 33, all the recording, correction, and data processing work was done by means of computers. The recording was done by our technical staff members Ms. Helga Ballmann, Ms. Mona El-Choura and Ms. Monika Kohl. Mr. Martin Schlotelburg and Mr. Ulrich Oberall supported our task by careful proofreading.