Abstract
GALAXIES at high redshift are very faint and difficult to study at optical and near-infrared wavelengths, but detection of far-infrared emission1 and molecular gas2,3 in a galaxy at redshift z≈2.3 has suggested that their early evolution may be investigated by these means instead. The host galaxies of quasars are promising candi-dates for these observations, particularly as quasars might be triggered by interactions and mergers between galaxies4,5 which result in dust- and gas-rich systems. The Cloverleaf, a gravitation-ally lensed quasar, has far-infrared/submillimetre emission indicat-ing a substantial dust content6, and therefore potentially a large amount of gas. Here we report the detection of carbon monoxide emission from the Cloverleaf, which we interpret as indicating a mass of molecular gas that is comparable to the total dynamical mass of the host galaxy, and which is consistent with the total baryonic content of a present-day luminous galaxy. This suggests that, although some processing of gas through stars has taken place in the Cloverleaf at a lookback time of 85% of the current age of the Universe, much of the future stellar content has yet to be formed.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Rowan-Robinson, M. et al. Nature 351, 719–721 (1991).
Brown, R. L. & Vanden Bout, P. A. Astrophys. J. 397, L19–L22 (1992).
Solomon, P. M., Downes, D. & Radford, S. J. E. Astrophys. J. 398, L29–L32 (1992).
Sanders, D. B. et al. Astrophys. J. 325, 74–91 (1988).
Hutchings, J. B. & Cambell, B. Nature 303, 584–588 (1983).
Barvainis, R., Antonucci, R. & Coleman, P. Astrophys. J. 399, L19–L22 (1992).
Magain, P. et al. Nature 334, 325–327 (1988).
Elston, R. et al. Astr. J. 107, 910–919 (1994).
Kayser, R. et al. Astrophys. J. 364, 15–22 (1990).
Downes, D. et al. Astrophys. J. 398, L25–L27 (1992).
Espey, B. R. Astrophys. J. 411, L59–L62 (1993).
Jakobsen, P. et al. Nature 370, 35–39 (1994).
Junkkarinen, V. T. in Active Galactic Nuclei (eds Osterbrock, D. E. & Miller, J. S.) 122 (Int. Astr. Un. Symp. No. 134, Kluwer, Dordrecht, 1989).
Hill, G. J., Thompson, K. L. & Elston, R. Astrophys. J. 414, L1–L4 (1993).
Sanders, D., Scoville, N. Z. & Soifer, B. T. Astrophys. J. 335, L1–L4 (1988).
Barvainis, R., Alloin, D. & Antonucci, R. Astrophys. J. 337, L69–L72 (1989).
Alloin, D., Barvainis, R., Gordon, M. & Antonucci, R. Astr. Astrophys. 265, 429–436 (1992).
Scoville, N. Z., Padin, S., Sanders, D. B., Soifer, B. T. & Yun, M. S. Astrophys. J. 415, L75–L77 (1993).
Barvainis, R. in Testing the AGN Paradigm (eds Holt, S. S., Neff, S. G. & Urry, C. M.) 129–138 (AIP, New York, 1992).
Antonucci, R. & Olszewski, E. W. Astr. J. 90, 2203–2206 (1985).
Barvainis, R. Nature 366, 298–299 (1993).
Antonucci, R. A. Rev. Astr. Astrophys. 31, 473–521 (1993).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Barvainis, R., Tacconi, L., Antonucci, R. et al. Extremely strong carbon monoxide emission from the Cloverleaf quasar at a redshift of 2.5. Nature 371, 586–588 (1994). https://doi.org/10.1038/371586a0
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1038/371586a0
This article is cited by
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.