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Identification of radio sources in clusters of galaxies. / Gubanov, A. G.; Reshetnikov, V. P.

In: Astronomy Letters, Vol. 25, No. 6, 01.06.1999, p. 380-388.

Research output: Contribution to journal › Article › peer-review

Harvard

Gubanov, AG & Reshetnikov, VP 1999, 'Identification of radio sources in clusters of galaxies', Astronomy Letters, vol. 25, no. 6, pp. 380-388.

APA

Gubanov, A. G., & Reshetnikov, V. P. (1999). Identification of radio sources in clusters of galaxies. Astronomy Letters, 25(6), 380-388.

Vancouver

Gubanov AG, Reshetnikov VP. Identification of radio sources in clusters of galaxies. Astronomy Letters. 1999 Jun 1;25(6):380-388.

Author

Gubanov, A. G. ; Reshetnikov, V. P. / Identification of radio sources in clusters of galaxies. In: Astronomy Letters. 1999 ; Vol. 25, No. 6. pp. 380-388.

BibTeX

@article{9f171d5e915143d18cb4203995952611,
title = "Identification of radio sources in clusters of galaxies",
abstract = "We have carried out a detailed identification of radio sources from the FIRST catalog lying within the Abell radii of 26 rich galactic clusters with optical objects in the APM and DSS surveys. Of the 326 radio sources in the cluster fields, 99 are identified, 40 have probable identifications, and 187 are unidentified. Among these last sources, 20 are definitely located in the clusters and 34 are cluster members with high probability. Thus, ≈30-40% of the FIRST radio sources could be identified using APM and DSS data, and, on the average, there were two sources in each cluster.",
author = "Gubanov, {A. G.} and Reshetnikov, {V. P.}",
year = "1999",
month = jun,
day = "1",
language = "English",
volume = "25",
pages = "380--388",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "6",

}

RIS

TY - JOUR

T1 - Identification of radio sources in clusters of galaxies

AU - Gubanov, A. G.

AU - Reshetnikov, V. P.

PY - 1999/6/1

Y1 - 1999/6/1

N2 - We have carried out a detailed identification of radio sources from the FIRST catalog lying within the Abell radii of 26 rich galactic clusters with optical objects in the APM and DSS surveys. Of the 326 radio sources in the cluster fields, 99 are identified, 40 have probable identifications, and 187 are unidentified. Among these last sources, 20 are definitely located in the clusters and 34 are cluster members with high probability. Thus, ≈30-40% of the FIRST radio sources could be identified using APM and DSS data, and, on the average, there were two sources in each cluster.

AB - We have carried out a detailed identification of radio sources from the FIRST catalog lying within the Abell radii of 26 rich galactic clusters with optical objects in the APM and DSS surveys. Of the 326 radio sources in the cluster fields, 99 are identified, 40 have probable identifications, and 187 are unidentified. Among these last sources, 20 are definitely located in the clusters and 34 are cluster members with high probability. Thus, ≈30-40% of the FIRST radio sources could be identified using APM and DSS data, and, on the average, there were two sources in each cluster.

UR - http://www.scopus.com/inward/record.url?scp=0033242644&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:0033242644

VL - 25

SP - 380

EP - 388

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 6

ER -

ID: 36179948