The radio galaxy RC J1148+0455

Y. N. Pariǐskiǐ; N. S. Soboleva; A. I. Kopylov; O. V. Verkhodanov; A. V. Temirova; O. P. Zhelenkova; J. Winn; A. Fletcher; B. Burke

doi:10.1134/1.20410

The radio galaxy RC J1148+0455

Y. N. Pariǐskiǐ, N. S. Soboleva, A. I. Kopylov, O. V. Verkhodanov, A. V. Temirova, O. P. Zhelenkova, J. Winn, A. Fletcher, B. Burke

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

Abstract

Based on data from the MIT-GB-VLA 4850-MHz survey, we investigate the radio structure of RC J1148+0455 with a steep radio spectrum “α = -1.04” from the COLD catalog. The radio source consists of two components, each having a complex structure. We analyze an optical identification of the source by using 6-m telescope images. The centroid of the radio source falls on a group of eight galaxies at a 24^m level in R.

Original language	English (US)
Pages (from-to)	423-427
Number of pages	5
Journal	Astronomy Letters
Volume	26
Issue number	7
DOIs	https://doi.org/10.1134/1.20410
State	Published - Jul 2000
Externally published	Yes

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Radio galaxies

Access to Document

10.1134/1.20410

Cite this

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title = "The radio galaxy RC J1148+0455",

abstract = "Based on data from the MIT-GB-VLA 4850-MHz survey, we investigate the radio structure of RC J1148+0455 with a steep radio spectrum “α = -1.04” from the COLD catalog. The radio source consists of two components, each having a complex structure. We analyze an optical identification of the source by using 6-m telescope images. The centroid of the radio source falls on a group of eight galaxies at a 24m level in R.",

keywords = "Radio galaxies",

author = "Pariǐskiǐ, {Y. N.} and Soboleva, {N. S.} and Kopylov, {A. I.} and Verkhodanov, {O. V.} and Temirova, {A. V.} and Zhelenkova, {O. P.} and J. Winn and A. Fletcher and B. Burke",

note = "Funding Information: ACKNOWLEDGMENTS This study was supported in part by the Russian Foundation for Basic Research (project nos. 99-07-90334 and 99-02-17114), as well as the Federal Program “Astronomy” (project nos. 1.2.1.2 and 1.2.2.4) and the Federal Program “Integration” (project no. 578).",

year = "2000",

month = jul,

doi = "10.1134/1.20410",

language = "English (US)",

volume = "26",

pages = "423--427",

journal = "Astronomy Letters",

issn = "1063-7737",

publisher = "Pleiades Publishing",

number = "7",

}

TY - JOUR

T1 - The radio galaxy RC J1148+0455

AU - Pariǐskiǐ, Y. N.

AU - Soboleva, N. S.

AU - Kopylov, A. I.

AU - Verkhodanov, O. V.

AU - Temirova, A. V.

AU - Zhelenkova, O. P.

AU - Winn, J.

AU - Fletcher, A.

AU - Burke, B.

N1 - Funding Information: ACKNOWLEDGMENTS This study was supported in part by the Russian Foundation for Basic Research (project nos. 99-07-90334 and 99-02-17114), as well as the Federal Program “Astronomy” (project nos. 1.2.1.2 and 1.2.2.4) and the Federal Program “Integration” (project no. 578).

PY - 2000/7

Y1 - 2000/7

N2 - Based on data from the MIT-GB-VLA 4850-MHz survey, we investigate the radio structure of RC J1148+0455 with a steep radio spectrum “α = -1.04” from the COLD catalog. The radio source consists of two components, each having a complex structure. We analyze an optical identification of the source by using 6-m telescope images. The centroid of the radio source falls on a group of eight galaxies at a 24m level in R.

AB - Based on data from the MIT-GB-VLA 4850-MHz survey, we investigate the radio structure of RC J1148+0455 with a steep radio spectrum “α = -1.04” from the COLD catalog. The radio source consists of two components, each having a complex structure. We analyze an optical identification of the source by using 6-m telescope images. The centroid of the radio source falls on a group of eight galaxies at a 24m level in R.

KW - Radio galaxies

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DO - 10.1134/1.20410

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VL - 26

SP - 423

EP - 427

JO - Astronomy Letters

JF - Astronomy Letters

IS - 7

ER -

The radio galaxy RC J1148+0455

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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