On the Jeans-mass in cosmology
Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mit...
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| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1991 |
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| Umfang: |
3 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: Astrophysics and space science - 1968, 181(1991) vom: Feb., Seite 323-325 |
| Übergeordnetes Werk: |
volume:181 ; year:1991 ; month:02 ; pages:323-325 ; extent:3 |
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| 520 | |a Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mitigated. | ||
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(DE-627)NLEJ193044676 DE-627 ger DE-627 rakwb eng On the Jeans-mass in cosmology 1991 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mitigated. Springer Online Journal Archives 1860-2002 Mészáros, A. oth Molnár, Z. oth in Astrophysics and space science 1968 181(1991) vom: Feb., Seite 323-325 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:181 year:1991 month:02 pages:323-325 extent:3 http://dx.doi.org/10.1007/BF00639098 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 181 1991 2 323-325 3 |
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(DE-627)NLEJ193044676 DE-627 ger DE-627 rakwb eng On the Jeans-mass in cosmology 1991 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mitigated. Springer Online Journal Archives 1860-2002 Mészáros, A. oth Molnár, Z. oth in Astrophysics and space science 1968 181(1991) vom: Feb., Seite 323-325 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:181 year:1991 month:02 pages:323-325 extent:3 http://dx.doi.org/10.1007/BF00639098 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 181 1991 2 323-325 3 |
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(DE-627)NLEJ193044676 DE-627 ger DE-627 rakwb eng On the Jeans-mass in cosmology 1991 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mitigated. Springer Online Journal Archives 1860-2002 Mészáros, A. oth Molnár, Z. oth in Astrophysics and space science 1968 181(1991) vom: Feb., Seite 323-325 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:181 year:1991 month:02 pages:323-325 extent:3 http://dx.doi.org/10.1007/BF00639098 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 181 1991 2 323-325 3 |
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(DE-627)NLEJ193044676 DE-627 ger DE-627 rakwb eng On the Jeans-mass in cosmology 1991 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mitigated. Springer Online Journal Archives 1860-2002 Mészáros, A. oth Molnár, Z. oth in Astrophysics and space science 1968 181(1991) vom: Feb., Seite 323-325 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:181 year:1991 month:02 pages:323-325 extent:3 http://dx.doi.org/10.1007/BF00639098 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 181 1991 2 323-325 3 |
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(DE-627)NLEJ193044676 DE-627 ger DE-627 rakwb eng On the Jeans-mass in cosmology 1991 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mitigated. Springer Online Journal Archives 1860-2002 Mészáros, A. oth Molnár, Z. oth in Astrophysics and space science 1968 181(1991) vom: Feb., Seite 323-325 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:181 year:1991 month:02 pages:323-325 extent:3 http://dx.doi.org/10.1007/BF00639098 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 181 1991 2 323-325 3 |
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in Astrophysics and space science 181(1991) vom: Feb., Seite 323-325 volume:181 year:1991 month:02 pages:323-325 extent:3 |
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Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mitigated. |
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Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mitigated. |
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Abstract The matter of the Universe after recombination is considered as an expanding gas. the Jeans-mass obtained for this gas may essentially be larger than it is usually expected. This means that the discrepancy between the theoretical Jeans-mass and the observed masses of the galaxies may be mitigated. |
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