Molecular outflow and feedback in the obscured quasar XID2028 revealed by ALMA

Autor: Emanuele Daddi, Filippo Fraternali, Rosita Paladino, Lorenzo Busoni, Paola Santini, Dieter Lutz, Marcella Brusa, Michele Perna, Mark Sargent, Giorgio Lanzuisi, Giovanni Cresci, Andrea Comastri, Alessandro Marconi, Sebastian Rabien, Fabrizio Fiore, Francesco Di Vito, Filippo Mannucci, Chiara Feruglio, Iskren Y. Georgiev, A. Bongiorno, N. Z. Scoville, Stefano Carniani, Marco Bonaglia, Enrico Piconcelli, Cristian Vignali, F. Duras, G. Zamorani, F. La Franca, Elisabeta Lusso, Viviana Casasola, Roberto Gilli, V. Mainieri
Přispěvatelé: Brusa, M., Cresci, G., Daddi, E., Paladino, R., Perna, MARIA FRANCESCA, Bongiorno, A., Lusso, E., Sargent, M. T., Casasola, V., Feruglio, C., Fraternali, Fabrizio, Georgiev, I., Mainieri, V., Carniani, S., Comastri, A., Duras, F., Fiore, F., Mannucci, F., Marconi, A., Piconcelli, E., Zamorani, G., Gilli, R., La Franca, F., Lanzuisi, G., Lutz, D., Santini, P., Scoville, N. Z., Vignali, C., DI VITO, Francesco, Rabien, S., Busoni, L., Bonaglia, M., Brusa M., Cresci G., Daddi E. , Paladino R., Perna M., Bongiorno A., Lusso E., Sargent M. T., Casasola V., Feruglio C., Fraternali F. , Georgiev I., Mainieri V., Carniani S., Comastri A., Duras F., Fiore F., Mannucci F., Marconi A., Piconcelli E., Zamorani G., Gilli R., La Franca F., Lanzuisi G., Lutz D., Santini P., Scoville N. Z., Vignali C., Vito F. , Rabien S., Busoni L., Bonaglia M., Perna, M., Fraternali, F., Vito, F., Carniani, Stefano [0000-0002-6719-380X], Apollo - University of Cambridge Repository, ITA, USA, GBR, FRA, DEU
Rok vydání: 2018
Předmět:
Zdroj: NASA Astrophysics Data System
Astronomy and Astrophysics
Astronomy & astrophysics, 2018, Vol.612, pp.A29 [Peer Reviewed Journal]
Astronomy & Astrophysics
ISSN: 0004-6361
Popis: We imaged, with ALMA and ARGOS/LUCI, the molecular gas and dust and stellar continuum in XID2028, which is an obscured quasi-stellar object (QSO) at z = 1.593, where the presence of a massive outflow in the ionised gas component traced by the [OIII]5007 emission has been resolved up to 10 kpc. This target represents a unique test case to study QSO feedback in action at the peak epoch of AGN-galaxy co-evolution. The QSO was detected in the CO(5 − 4) transition and in the 1.3 mm continuum at ~30 and ~20σ significance, respectively; both emissions are confined in the central (
Includes STFC and ERC grants.
Databáze: OpenAIRE