1. |
Can the ten‐dimensional phase prior to Calabi‐Yau splitting of the super‐string phase generate the primordial entropy of the universe? |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 1-4
C. Wolf,
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摘要:
AbstractIt is shown that the primordial entropy of the universe can be generated in the residual phase prior to Calabi‐Yau splitting and following the passing to the field theory limit of the heterotic super‐string in ten space‐time dimensions, wherein matter is represented by either a radiative equation of state or the equation of state for stiff m
ISSN:0004-6337
DOI:10.1002/asna.2113110102
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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2. |
Catalogue of non‐Abell clusters of galaxies with published photometric data |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 5-30
F. W. Baier,
R. Ziener,
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摘要:
AbstractThis catalogue is a compilation of references of publications with photometric data in and around non‐Abell clusters of galaxie
ISSN:0004-6337
DOI:10.1002/asna.2113110103
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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3. |
Absolute proper motions of blue objects in the vicinity of M33 |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 31-34
G. A. Richter,
R.‐D. Scholz,
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摘要:
Abstract36 objects with mainly negative (U—B) indices were investigated for variability and proper motions. 10 objects with significant or suspected proper motions and 8 variable objects were detected. Using these criteria, it was possible to separate white dwarfs from quasi‐stellar objects to some ext
ISSN:0004-6337
DOI:10.1002/asna.2113110104
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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4. |
Three‐dimensional distribution of high‐velocity stars |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 35-39
J. Greiner,
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摘要:
AbstractNumerical calculations support the conjecture that high velocity stars born in or near the rotating disk are not distributed spherically throughout the galaxy. Instead an empty funnel region forms around the rotation axis of the galaxy, where no stars reside. The funnel appears only for high velocity stars, such as old pulsars. Within about 50 kpc distance from the galactic center the funnel shape is almost not dependent on the existence of a massive corona.
ISSN:0004-6337
DOI:10.1002/asna.2113110105
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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5. |
J. H. DAVENPORT, Y. LIRET, E. TOURNIER: Computer Algcbm. Systems and Algorithms for Algebraic Computation. Academic Press, London, San Diego, New York, Boston, Sydney, Tokyo, Toronto 1988. 267 Seiten. Preis: £ 14,‐. ISBN 0‐12‐204230‐1 |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 39-39
Manfred Schulrz,
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ISSN:0004-6337
DOI:10.1002/asna.2113110106
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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6. |
D. B. MELROSE: Instabilities in Space and Laboratory Plasmas. Cambridge University Press, Cambridge, 1986. XII + 280 S. Preis: US‐$ 49,50. ISBN 0‐521‐30541‐1 |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 40-40
B. Kliem,
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ISSN:0004-6337
DOI:10.1002/asna.2113110107
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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7. |
Magnetic field and radial velocity of the Ap star 52 Her. I. Observations, measurements, results |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 41-48
E. Gerth,
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摘要:
AbstractSince 1971 the magnetic Ap star 52 Her has been investigated with respect to its magnettic field and radial velocity on the observational basis of 140 photographic Zeeman spectrograms obtained at the 2m‐telescope in Tautenburg. Additionally, 47 normal spectrograms were used for the determination of the radial velocity only. The technical foundation for observation and measurement is considered. The main purpose of the paper, however, is the documentation of the observations and the measuring results. Deductions drawn from the material assorted here or taken from other sources are put off to following paper
ISSN:0004-6337
DOI:10.1002/asna.2113110108
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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8. |
Turbulence influenced line formation in stellar atmospheres |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 49-53
J. Stahlberg,
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摘要:
AbstractThe influence of stochastic velocity fields with finite correlation lengths on the formation of spectral lines is taken into account without restrictions to specific velocity models. To construct a perturbation theory treating the influence of stochastic motion on the radiative transfer we start with the stochastic transfer equation for plane‐parallel atmospheres and expand it to an infinite hierarchical system. An appropriate cut‐off of the infinite system admits to achieve exactly the micro‐ and macroturbulent limit at every level of approach. The formalism is derived forn‐point correlations of the absorption coefficient and specialised for 2‐point cor
ISSN:0004-6337
DOI:10.1002/asna.2113110109
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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9. |
F. MELCHIORRI, L. MAIANI (eds.): Tbe Cosmic Background Radiation and Fundamental Physics. Conference Proceedings. Third Rome Meeting on Astrophysics. Italian Physical Society, Bologna, 1985, XII + 291 Seiten. |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 54-54
Volker Müller,
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ISSN:0004-6337
DOI:10.1002/asna.2113110111
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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10. |
A survey of the peculiar radio emission of the solar behind‐limb event on 16th February 1984 |
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Astronomische Nachrichten,
Volume 311,
Issue 1,
1990,
Page 55-62
I. M. Chertok,
V. V. Fomichev,
R. V. Gorgutsa,
A. K. Markeev,
T. S. Podstrigach,
H. Aurass,
J. Hildebrandt,
B. Kliem,
A. Krüger,
J. Kurths,
M. KarlickýA,
A. Tlamicha,
H. W. Urbarz,
P. Zlobec,
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摘要:
AbstractBasing on radio measurements from different stations the paper presents a compilation of observations and resultinng questions concerning the interpretation of some remarkable features of the solar behind‐limb event on 16th February 1984. The event was related to a very strong relativistic particle emission. Attention is paid to the related microwave radiation stimulating a discussion of the discrimination between plasma and gyromagnetic radiation being important for plasma diagnostics. Another outstanding feature is the occurrence of a spectacular multi‐band U‐shaped type II burst pattern challenging a discussion of possible higher harmonic plasma radi
ISSN:0004-6337
DOI:10.1002/asna.2113110112
出版商:WILEY‐VCH Verlag
年代:1990
数据来源: WILEY
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