ISO far-infrared observations of rich galaxy clusters I. Abell 2670

Lene Hansen, H.E. Jorgensen, Hans Ulrik Nørgaard-Nielsen, Kenneth Pedersen, P. Goudfrooij, M.J.D. Linden-Vornle

Research output: Contribution to journalJournal articleResearchpeer-review

Abstract

As part of an investigation of far-infrared emission from rich galaxy clusters the central part of Abell 2670 has been mapped with ISO at 60 mu m, 100 mu m, 135 mu m, and 200 mu m using the PHT-C camera. Point sources detected in the field have infrared fluxes comparable to normal spirals at the cluster distance. Probable optical counterparts are cluster galaxies with various characteristics such as blue colour, Ha emission, or double nuclei. One source is extended which could possibly be emission from intracluster dust in debris from spiral galaxies.
Original languageEnglish
JournalAstronomy and Astrophysics
Volume349
Issue number2
Pages (from-to)406-410
ISSN0004-6361
Publication statusPublished - 1999

Keywords

  • galaxies : clusters : individual : Abell 2670
  • infrared : galaxies

Cite this

Hansen, L., Jorgensen, H. E., Nørgaard-Nielsen, H. U., Pedersen, K., Goudfrooij, P., & Linden-Vornle, M. J. D. (1999). ISO far-infrared observations of rich galaxy clusters I. Abell 2670. Astronomy and Astrophysics, 349(2), 406-410.
Hansen, Lene ; Jorgensen, H.E. ; Nørgaard-Nielsen, Hans Ulrik ; Pedersen, Kenneth ; Goudfrooij, P. ; Linden-Vornle, M.J.D. / ISO far-infrared observations of rich galaxy clusters I. Abell 2670. In: Astronomy and Astrophysics. 1999 ; Vol. 349, No. 2. pp. 406-410.
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abstract = "As part of an investigation of far-infrared emission from rich galaxy clusters the central part of Abell 2670 has been mapped with ISO at 60 mu m, 100 mu m, 135 mu m, and 200 mu m using the PHT-C camera. Point sources detected in the field have infrared fluxes comparable to normal spirals at the cluster distance. Probable optical counterparts are cluster galaxies with various characteristics such as blue colour, Ha emission, or double nuclei. One source is extended which could possibly be emission from intracluster dust in debris from spiral galaxies.",
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year = "1999",
language = "English",
volume = "349",
pages = "406--410",
journal = "Astronomy & Astrophysics",
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Hansen, L, Jorgensen, HE, Nørgaard-Nielsen, HU, Pedersen, K, Goudfrooij, P & Linden-Vornle, MJD 1999, 'ISO far-infrared observations of rich galaxy clusters I. Abell 2670', Astronomy and Astrophysics, vol. 349, no. 2, pp. 406-410.

ISO far-infrared observations of rich galaxy clusters I. Abell 2670. / Hansen, Lene; Jorgensen, H.E.; Nørgaard-Nielsen, Hans Ulrik; Pedersen, Kenneth; Goudfrooij, P.; Linden-Vornle, M.J.D.

In: Astronomy and Astrophysics, Vol. 349, No. 2, 1999, p. 406-410.

Research output: Contribution to journalJournal articleResearchpeer-review

TY - JOUR

T1 - ISO far-infrared observations of rich galaxy clusters I. Abell 2670

AU - Hansen, Lene

AU - Jorgensen, H.E.

AU - Nørgaard-Nielsen, Hans Ulrik

AU - Pedersen, Kenneth

AU - Goudfrooij, P.

AU - Linden-Vornle, M.J.D.

PY - 1999

Y1 - 1999

N2 - As part of an investigation of far-infrared emission from rich galaxy clusters the central part of Abell 2670 has been mapped with ISO at 60 mu m, 100 mu m, 135 mu m, and 200 mu m using the PHT-C camera. Point sources detected in the field have infrared fluxes comparable to normal spirals at the cluster distance. Probable optical counterparts are cluster galaxies with various characteristics such as blue colour, Ha emission, or double nuclei. One source is extended which could possibly be emission from intracluster dust in debris from spiral galaxies.

AB - As part of an investigation of far-infrared emission from rich galaxy clusters the central part of Abell 2670 has been mapped with ISO at 60 mu m, 100 mu m, 135 mu m, and 200 mu m using the PHT-C camera. Point sources detected in the field have infrared fluxes comparable to normal spirals at the cluster distance. Probable optical counterparts are cluster galaxies with various characteristics such as blue colour, Ha emission, or double nuclei. One source is extended which could possibly be emission from intracluster dust in debris from spiral galaxies.

KW - galaxies : clusters : individual : Abell 2670

KW - infrared : galaxies

M3 - Journal article

VL - 349

SP - 406

EP - 410

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

IS - 2

ER -

Hansen L, Jorgensen HE, Nørgaard-Nielsen HU, Pedersen K, Goudfrooij P, Linden-Vornle MJD. ISO far-infrared observations of rich galaxy clusters I. Abell 2670. Astronomy and Astrophysics. 1999;349(2):406-410.