Frequency-dependence of the statistics of radio sources
Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the...
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| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1985 |
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| Umfang: |
12 |
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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: Jan., Seite 125-136 |
| Übergeordnetes Werk: |
volume:108 ; year:1985 ; month:01 ; pages:125-136 ; extent:12 |
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NLEJ193006677 |
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| 520 | |a Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the class of doubles whose visible parameters depend on their spatial orientation being relative to the observer. | ||
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(DE-627)NLEJ193006677 DE-627 ger DE-627 rakwb eng Frequency-dependence of the statistics of radio sources 1985 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the class of doubles whose visible parameters depend on their spatial orientation being relative to the observer. Springer Online Journal Archives 1860-2002 Amirkhanyan, V. R. oth in Astrophysics and space science 1968 108(1985) vom: Jan., Seite 125-136 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:108 year:1985 month:01 pages:125-136 extent:12 http://dx.doi.org/10.1007/BF00650124 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 108 1985 1 125-136 12 |
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(DE-627)NLEJ193006677 DE-627 ger DE-627 rakwb eng Frequency-dependence of the statistics of radio sources 1985 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the class of doubles whose visible parameters depend on their spatial orientation being relative to the observer. Springer Online Journal Archives 1860-2002 Amirkhanyan, V. R. oth in Astrophysics and space science 1968 108(1985) vom: Jan., Seite 125-136 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:108 year:1985 month:01 pages:125-136 extent:12 http://dx.doi.org/10.1007/BF00650124 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 108 1985 1 125-136 12 |
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(DE-627)NLEJ193006677 DE-627 ger DE-627 rakwb eng Frequency-dependence of the statistics of radio sources 1985 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the class of doubles whose visible parameters depend on their spatial orientation being relative to the observer. Springer Online Journal Archives 1860-2002 Amirkhanyan, V. R. oth in Astrophysics and space science 1968 108(1985) vom: Jan., Seite 125-136 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:108 year:1985 month:01 pages:125-136 extent:12 http://dx.doi.org/10.1007/BF00650124 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 108 1985 1 125-136 12 |
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(DE-627)NLEJ193006677 DE-627 ger DE-627 rakwb eng Frequency-dependence of the statistics of radio sources 1985 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the class of doubles whose visible parameters depend on their spatial orientation being relative to the observer. Springer Online Journal Archives 1860-2002 Amirkhanyan, V. R. oth in Astrophysics and space science 1968 108(1985) vom: Jan., Seite 125-136 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:108 year:1985 month:01 pages:125-136 extent:12 http://dx.doi.org/10.1007/BF00650124 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 108 1985 1 125-136 12 |
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(DE-627)NLEJ193006677 DE-627 ger DE-627 rakwb eng Frequency-dependence of the statistics of radio sources 1985 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the class of doubles whose visible parameters depend on their spatial orientation being relative to the observer. Springer Online Journal Archives 1860-2002 Amirkhanyan, V. R. oth in Astrophysics and space science 1968 108(1985) vom: Jan., Seite 125-136 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:108 year:1985 month:01 pages:125-136 extent:12 http://dx.doi.org/10.1007/BF00650124 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 108 1985 1 125-136 12 |
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in Astrophysics and space science 108(1985) vom: Jan., Seite 125-136 volume:108 year:1985 month:01 pages:125-136 extent:12 |
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frequency-dependence of the statistics of radio sources |
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Frequency-dependence of the statistics of radio sources |
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Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the class of doubles whose visible parameters depend on their spatial orientation being relative to the observer. |
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Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the class of doubles whose visible parameters depend on their spatial orientation being relative to the observer. |
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Abstract Without assuming the existence of two populations of radio sources, the counts of vs frequency, spectral index vs flux density, and counts vs spectral index dependences have been derived. An assumption —with arguments to support it—is made that most extragalactic radio sources belong to the class of doubles whose visible parameters depend on their spatial orientation being relative to the observer. |
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Frequency-dependence of the statistics of radio sources |
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