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...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Amirkhanyan, V. R. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1985 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1985 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 108(1985), 1 vom: Jan., Seite 125-136 |
|---|---|
| Übergeordnetes Werk: |
volume:108 ; year:1985 ; number:1 ; month:01 ; pages:125-136 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00650124 |
|---|
| Katalog-ID: |
OLC2066154806 |
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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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| 650 | 4 | |a Index Dependence | |
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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. © D. Reidel Publishing Company 1985 |
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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. © D. Reidel Publishing Company 1985 |
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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. © D. Reidel Publishing Company 1985 |
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Frequency-dependence of the statistics of radio sources |
| url |
https://doi.org/10.1007/BF00650124 |
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false |
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129062723 |
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| doi_str |
10.1007/BF00650124 |
| up_date |
2024-07-04T03:52:52.875Z |
| _version_ |
1803619058722013184 |
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