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:	Amirkhanyan, V. R. [verfasserIn]

Format:	Artikel
Sprache:	Englisch

Erschienen:	1985

Schlagwörter:	Flux Density Spectral Index Radio Source Density Region Flux Density Region

Anmerkung:	© D. Reidel Publishing Company 1985

Übergeordnetes Werk:	Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 108(1985), 2 vom: Jan., Seite 319-322
Übergeordnetes Werk:	volume:108 ; year:1985 ; number:2 ; month:01 ; pages:319-322

Links:	Volltext

DOI / URN:	10.1007/BF01068258

Katalog-ID:	OLC2066155012

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title_sort	the form of logn-logs relation in the domain of strong flux densities
title_auth	The form of logN-logS relation in the domain of strong flux densities
abstract	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. © D. Reidel Publishing Company 1985
abstractGer	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. © D. Reidel Publishing Company 1985
abstract_unstemmed	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. © D. Reidel Publishing Company 1985
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The form of logN-logS relation in the domain of strong flux densities

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