Fingerprint
Dive into the research topics of 'Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift'. Together they form a unique fingerprint.- Sort by
- Weight
- Alphabetically
Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift
B. H C Emonts*, M. D. Lehnert, M. Villar-Martín, R. P. Norris, R. D. Ekers, G. A. Van Moorsel, H. Dannerbauer, L. Pentericci, G. K. Miley, J. R. Allison, E. M. Sadler, P. Guillard, C. L. Carilli, M. Y. Mao, H. J A Röttgering, C. De Breuck, N. Seymour, B. Gullberg, D. Ceverino, P. Jagannathan
*Corresponding author for this work
- Centro de Astrobiología (INTA-CSIC)
- Institut de la Vision
- Universidad Autonoma de Madrid
- Australia Telescope National Facility
- Western Sydney University
- National Radio Astronomy Observatory Socorro
- Instituto de Astrofísica de Canarias
- Universidad de la Laguna
- Institut für Astrophysik
- Universitat Wien
- INAF-Osservatorio Astronomico di Roma
- Leiden Observatory Research Institute
- Sydney Institute for Astronomy
- University of Sydney
- University of Cambridge
- JIVE (Joint Institute for Very Long Baseline Interferometry in Europe)
- European Research Infrastructure Consortium
- European Southern Observatory (ESO)
- International Centre for Radio Astronomy Research (ICRAR)
- Curtin University
- Centre for Extragalactic Astronomy
- University of Durham
- Ruprecht-Karls Universitat Heidelberg - University of Heidelberg
Research output: Contribution to journal › Article › peer-review