Nature Communications (Aug 2022)
Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913
- M. Ginolfi,
- E. Piconcelli,
- L. Zappacosta,
- G. C. Jones,
- L. Pentericci,
- R. Maiolino,
- A. Travascio,
- N. Menci,
- S. Carniani,
- F. Rizzo,
- F. Arrigoni Battaia,
- S. Cantalupo,
- C. De Breuck,
- L. Graziani,
- K. Knudsen,
- P. Laursen,
- V. Mainieri,
- R. Schneider,
- F. Stanley,
- R. Valiante,
- A. Verhamme
Affiliations
- M. Ginolfi
- European Southern Observatory
- E. Piconcelli
- INAF—Osservatorio Astronomico di Roma
- L. Zappacosta
- INAF—Osservatorio Astronomico di Roma
- G. C. Jones
- Department of Physics, University of Oxford
- L. Pentericci
- INAF—Osservatorio Astronomico di Roma
- R. Maiolino
- Cavendish Laboratory, University of Cambridge
- A. Travascio
- Department of Physics, University of Milan Bicocca
- N. Menci
- INAF—Osservatorio Astronomico di Roma
- S. Carniani
- Scuola Normale Superiore
- F. Rizzo
- Cosmic Dawn Center (DAWN)
- F. Arrigoni Battaia
- Max-Planck-Institut für Astrophysik
- S. Cantalupo
- Department of Physics, University of Milan Bicocca
- C. De Breuck
- European Southern Observatory
- L. Graziani
- Dipartimento di Fisica, Sapienza, Universita di Roma
- K. Knudsen
- Department of Space, Earth, and Environment, Chalmers University of Technology, Onsala Space Observatory
- P. Laursen
- Cosmic Dawn Center (DAWN)
- V. Mainieri
- European Southern Observatory
- R. Schneider
- Dipartimento di Fisica, Sapienza, Universita di Roma
- F. Stanley
- Sorbonne Université, UPMC Université Paris 6 & CNRS, UMR 7095, Institut d’Astrophysique de Paris
- R. Valiante
- INAF—Osservatorio Astronomico di Roma
- A. Verhamme
- Observatoire de Genéve, Université de Genève
- DOI
- https://doi.org/10.1038/s41467-022-32297-x
- Journal volume & issue
-
Vol. 13,
no. 1
pp. 1 – 15
Abstract
Lyman-alpha emission is one of the observational probes for the high-redshift universe. Here, the authors show several Lyman-alpha emitting companion galaxies around the hot dust-obscured galaxy W0410-091 suggesting that the galaxy evolves in a very dense environment.
