Skip to content

Deep and narrow CO absorption revealing molecular clouds in the Hydra-A brightest cluster galaxy

Research output: Contribution to journalArticle (Academic Journal)

  • Tom Rose
  • A. C. Edge
  • F. Combes
  • M. Gaspari
  • S. Hamer
  • N. Nesvadba
  • H. Russell
  • G. R. Tremblay
  • S. A. Baum
  • C. O'Dea
  • A. B. Peck
  • C. Sarazin
  • A. Vantyghem
  • M. Bremer
  • M. Donahue
  • A. C. Fabian
  • G. Ferland
  • B. R. McNamara
  • R. Mittal
  • J. B. R. Oonk
  • P. Salomé
  • A. M. Swinbank
  • M. Voit
Original languageEnglish
Pages (from-to)229-238
JournalMonthly Notices of the Royal Astronomical Society
Issue number1
Early online date11 Feb 2019
DateAccepted/In press - 5 Feb 2019
DateE-pub ahead of print - 11 Feb 2019
DatePublished (current) - 1 May 2019


Active galactic nuclei play a crucial role in the accretion and ejection of gas in galaxies. Although their outflows are well studied, finding direct evidence of accretion has proved very difficult and has so far been done for very few sources. A promising way to study the significance of cold accretion is by observing the absorption of an active galactic nucleus's extremely bright radio emission by the cold gas lying along the line of sight. As such, we present ALMA CO(1-0) and CO(2-1) observations of the Hydra-A brightest cluster galaxy (z = 0.054) which reveal the existence of cold, molecular gas clouds along the line of sight to the galaxy's extremely bright and compact mm-continuum source. They have apparent motions relative to the central supermassive black hole of between -43 and -4 km s-1 and are most likely moving along stable, low ellipticity orbits. The identified clouds form part of a ˜109 M⊙, approximately edge-on disc of cold molecular gas. With peak CO(2-1) optical depths of τ = 0.88 ^{+0.06}_{-0.06}, they include the narrowest and by far the deepest absorption of this type which has been observed to date in a brightest cluster galaxy. By comparing the relative strengths of the lines for the most strongly absorbing region, we are able to estimate a gas temperature of 42^{+25}_{-11} K and line of sight column densities of N_{CO}=2^{+3}_{-1}× 10 ^{17} {cm}^{-2} and N_{H2 }=7^{+10}_{-4}× 10 ^{20} {cm}^{-2}.

    Research areas

  • galaxies: clusters: individual: Hydra-A, galaxies: ISM, radio lines: galaxies

Download statistics

No data available



  • Full-text PDF (final published version)

    Rights statement: This is the final published version of the article (version of record). It first appeared online via OUP at . Please refer to any applicable terms of use of the publisher.

    Final published version, 1.22 MB, PDF document

    Licence: Other



View research connections

Related faculties, schools or groups