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1. |
The asymmetry of the Coma cluster of galaxies |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 89-97
F. W. Baier,
K. Fritze,
H. Tiersch,
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摘要:
AbstractA detailed reinvestigation of the Coma cluster basing on enlarged observational material of number density distributions and radial velocities of galaxies as well as radio and x‐ray data is performed and supports our previous conclusion that this cluster possesses a substructure. This substructure is in the south‐western region of the cluster and produces the impression of an elongated cluster structure in the direction of the bridge between Coma and A 1367. A 1656 seems to be a cD‐like cluster with NGC 4874 as the only dominating giant central g
ISSN:0004-6337
DOI:10.1002/asna.2113110202
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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2. |
NORBERT STRAUMANN: Allgemeine Relativitätstheorie und relativistische Astrophysik. Zweite, korrigierte und erweiterte Auflage. Lecture Notes in Physics No. 150. Springer‐Verlag Berlin, Heidelberg, New York, 1988, VIII + 491 Seiten. Preis: DM 62,50. ISBN 3‐540‐18763‐4. |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 98-98
Volker Müller,,
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ISSN:0004-6337
DOI:10.1002/asna.2113110204
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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3. |
The massive scalar field in a closed Friedmann universe model — new rigorous results |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 99-105
H.‐J. Schmidt,
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摘要:
AbstractFor the minimally coupled scalar field in Einstein's theory of gravitation we look for the space of solutions within the class of closed Friedmann universe models. We proveD≥ 1, whereD≥ is the dimension of the set of solutions which can be integrated up tot→ ∞ (D>0 was conjectured by PAGE(1984)). We discuss concepts like “the probability of the appearance of a sufficiently long inflationary phase” and argue that it is primarily a probability measure μ in the spaceVof solutions (and not in the space of initial conditions) which has to be applied. μ is naturally defined for Bianchi‐type I cosmological models becauseVis a compact cube. The problems with the closed Friedmann model (which led to controversial claims in the literature) will be shown to originate from the fact thatVhas a complicated non‐compact non‐Hausdorff Geroch topology: no natural definition of μ can be given.We conclude: the present state of our universe can be explained by models of the type discussed, but thereby the anthropic principle cannot b
ISSN:0004-6337
DOI:10.1002/asna.2113110205
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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4. |
KEN'CHI NOMOTO (Ed.): Atmospheric Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion (Proceedings of the 108th IAU‐Colloquium, Tokyo 1987). Lecture Notes in Physics, Bd. 305. Springer‐Verlag, Berlin/Heidelberg/New York/London/Paris/Tokyo, 1988. 484 Seiten, Preis: DM 80.‐.ISBN 3‐540‐1 9478‐9 Berlin/Heidelberg/New York ISBN 0‐387‐19478‐9 New York/Berlin/Heidelberg |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 106-106
Jürgen Stahlberg,
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ISSN:0004-6337
DOI:10.1002/asna.2113110207
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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5. |
Diffussion of a scalar field in a compressible turbulent medium |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 107-116
N. A. Silant'Ev,
M. D. Korolkov,
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摘要:
AbstractThe diffusion of scalar fields (temperature, density number of some admixture) in a compressible medium showing an isotropic, homogeneous and stationary turbulence is considered. The derived formulae for turbulent diffusivity χT(ξ) hold up to ξ ≈ 1, where ξ =u0τ0/R0(u0, τ0, andR0are characteristic velocity, life‐time, and correlation length of turbulent pulsations, respectively. The velocity field of turbulent motionsu(r, t) is assumed to be known and the influence of the scalar field ontou(r, t) is neglected. It is shown that the velocity correlators, which change their signs in dependence on the space corrdinates, may give negative values for ξT(ξ)
ISSN:0004-6337
DOI:10.1002/asna.2113110208
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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6. |
Photographic measurements of 320 double stars of POURTEAUremeasured 50 years after their discovery |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 117-121
D. Gellera,
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摘要:
AbstractThe position angle and separation of 320 double stars from Pourteau's Catalogue (18h<α<19h) measured on the prints of the Palomar Observatory Sky Survey 50 years after their discovery are given
ISSN:0004-6337
DOI:10.1002/asna.2113110209
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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7. |
Buchbesprechung |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 122-122
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ISSN:0004-6337
DOI:10.1002/asna.2113110210
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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8. |
Beobachtungen Kleiner Planeten. IX |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 123-131
F. Börngen,
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摘要:
AbstractEs wird eine Übersicht über die im Jahr 1988 auf Tautenburger Schmidtplatten gefundenen Kleinen Planeten gegeben. 386 Objekte wurden entdeckt und für diese 1218 Positionen gerechnet. Es handelt sich um 87 numerierte Objekte sowie um 299 Planetoiden mit provisorischer Bezeichnung. Unter letzteren sind 252 neue Bezeichnungen. Für 40 im Berichtszeitraum numerierte Planeten haben Tautenburger Beobachtungen einen Beitrag geleistet. Darunter sind acht in Tautenburg entdeckte Planetoi
ISSN:0004-6337
DOI:10.1002/asna.2113110211
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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9. |
B. STEPHENSON: Kepler's physical astronomy. Studies in the History of Mathematics and Physical Sciences, Vol. 13. Springer‐Verlag New York, Berlin, Heidelberg. London. Paris, Tokyo 1987, 217 Seiten. Preis: DM 118,‐. ISBN 0‐387‐96541‐6 |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 132-132
Hans‐Joachim Felber,
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ISSN:0004-6337
DOI:10.1002/asna.2113110213
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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10. |
Simple methods for orbit determination and identification of asteroids. I |
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Astronomische Nachrichten,
Volume 311,
Issue 2,
1990,
Page 133-136
L. K. Kristensen,
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摘要:
AbstractThe many discoveries of main belt asteroids with insufficient observations for reliable orbits cause special difficulties for identifications and data storage; mainly because of the mixing of objects due to their motion in α and δ. This problem may be reduced by substituting positions by slowly and smoothly varying quantities. A rational system of preliminary designations will be proposed, and surveys and compact ephemerides are discussed. All computations are very simple and performed on a small, programmable pocket compute
ISSN:0004-6337
DOI:10.1002/asna.2113110214
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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