Dust in 3C 324

P. N. Best, H. J.A. Röttgering, M. N. Bremer, A. Cimatti, K. H. Mack, G. K. Miley, L. Pentericci, R. P.J. Tilanus, P. P. Van Der Werf

Research output: Contribution to journalArticlepeer-review

18 Scopus citations


The results of a deep submillimetre observation using SCUBA of the powerful radio galaxy 3C 324, at redshift z = 1.206, are presented. At 850 μm, emission from the location of the host radio galaxy is marginally detected at the 4.2σ level, 3.01 ± 0.72 mJy, but there is no detection of emission at 450 μm to a 3σ limit of 21 mJy. A new 32-GHz radio observation using the Effelsberg 100-m telescope confirms that the submillimetre signal is not associated with synchrotron emission. These observations indicate that both the mass of warm dust within 3C 324 and the star formation rate lie up to an order of magnitude below the values recently determined for radio galaxies at z ∼ 3-4. The results are compared with dust masses and star formation rates derived in other ways for 3C 324.

Original languageEnglish (US)
Pages (from-to)L15-L19
JournalMonthly Notices of the Royal Astronomical Society
Issue number1
StatePublished - Nov 21 1998
Externally publishedYes


  • Dust, extinction
  • Galaxies: ISM
  • Galaxies: active
  • Galaxies: individual: 3C 324
  • Radio continuum: galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


Dive into the research topics of 'Dust in 3C 324'. Together they form a unique fingerprint.

Cite this