The form of logN-logS relation in the domain of strong flux densities
Abstract The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices.
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1985 |
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| Umfang: |
4 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: Astrophysics and space science - 1968, 108(1985) vom: Feb., Seite 319-322 |
| Übergeordnetes Werk: |
volume:108 ; year:1985 ; month:02 ; pages:319-322 ; extent:4 |
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| 520 | |a Abstract The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices. | ||
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(DE-627)NLEJ193006804 DE-627 ger DE-627 rakwb eng The form of logN-logS relation in the domain of strong flux densities 1985 4 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices. Springer Online Journal Archives 1860-2002 Amirkhanyan, V. R. oth in Astrophysics and space science 1968 108(1985) vom: Feb., Seite 319-322 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:108 year:1985 month:02 pages:319-322 extent:4 http://dx.doi.org/10.1007/BF01068258 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 108 1985 2 319-322 4 |
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(DE-627)NLEJ193006804 DE-627 ger DE-627 rakwb eng The form of logN-logS relation in the domain of strong flux densities 1985 4 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices. Springer Online Journal Archives 1860-2002 Amirkhanyan, V. R. oth in Astrophysics and space science 1968 108(1985) vom: Feb., Seite 319-322 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:108 year:1985 month:02 pages:319-322 extent:4 http://dx.doi.org/10.1007/BF01068258 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 108 1985 2 319-322 4 |
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(DE-627)NLEJ193006804 DE-627 ger DE-627 rakwb eng The form of logN-logS relation in the domain of strong flux densities 1985 4 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices. Springer Online Journal Archives 1860-2002 Amirkhanyan, V. R. oth in Astrophysics and space science 1968 108(1985) vom: Feb., Seite 319-322 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:108 year:1985 month:02 pages:319-322 extent:4 http://dx.doi.org/10.1007/BF01068258 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 108 1985 2 319-322 4 |
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(DE-627)NLEJ193006804 DE-627 ger DE-627 rakwb eng The form of logN-logS relation in the domain of strong flux densities 1985 4 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices. Springer Online Journal Archives 1860-2002 Amirkhanyan, V. R. oth in Astrophysics and space science 1968 108(1985) vom: Feb., Seite 319-322 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:108 year:1985 month:02 pages:319-322 extent:4 http://dx.doi.org/10.1007/BF01068258 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 108 1985 2 319-322 4 |
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the form of logn-logs relation in the domain of strong flux densities |
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The form of logN-logS relation in the domain of strong flux densities |
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Abstract The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices. |
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Abstract The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices. |
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Abstract The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices. |
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