Zobrazeno 1 - 10
of 70
pro vyhledávání: '"F. Arrigoni Battaia"'
Autor:
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
Publikováno v:
Nature Communications, Vol 13, Iss 1, Pp 1-15 (2022)
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
Externí odkaz:
https://doaj.org/article/ea7346be48844af7a9cbe32579f2e85d
Autor:
E Iani, A Zanella, J Vernet, J Richard, M Gronke, F Arrigoni-Battaia, A Bolamperti, K I Caputi, A Humphrey, G Rodighiero, P Rinaldi, E Vanzella
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, ⟨10.1093/mnras/stac3198⟩
Monthly Notices of the Royal Astronomical Society, 518(4), 5018-5035. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 2022, ⟨10.1093/mnras/stac3198⟩
Monthly Notices of the Royal Astronomical Society, 518(4), 5018-5035. Oxford University Press
The origin of the Lyman-${\alpha}$ (Ly${\alpha}$) emission in galaxies is a long-standing issue: despite several processes known to originate this line (e.g. AGN, star formation, cold accretion, shock heating), it is difficult to discriminate among t
Autor:
F. Arrigoni Battaia, A. Obreja, C.-C. Chen, M. Nowotka, M. Fumagalli, J.X. Prochaska, Y. Yang, Z. Cai, N. Munoz-Elgueta, M. Fossati
Publikováno v:
Astronomy & Astrophysics.
Autor:
A Girdhar, C M Harrison, V Mainieri, A Bittner, T Costa, P Kharb, D Mukherjee, F Arrigoni Battaia, D M Alexander, G Calistro Rivera, C Circosta, C De Breuck, A C Edge, E P Farina, D Kakkad, G B Lansbury, S J Molyneux, J R Mullaney, Silpa S, A P Thomson, S R Ward
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2022, Vol.512(2), pp.1608-1628 [Peer Reviewed Journal]
We present a study of a luminous, z=0.15, type-2 quasar (log [L([OIII])/(erg/s)]=42.8) from the Quasar Feedback Survey. It is classified as 'radio-quiet' (log [L(1.4 GHz)/(W/Hz)]=23.8); however, radio imaging reveals ~1 kpc low-power jets (log [Pjet/
Autor:
H R Stacey, F Arrigoni Battaia
We present deep observations of CO(3-2) from the Cloverleaf lensed quasar-starburst at $z=2.56$. We discover a 4-5 times less massive companion at a projected distance of 33 kpc from the Cloverleaf host galaxy. The galaxies are connected by a bridge
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e8487fb2354774c0cadb908f634f34a
http://arxiv.org/abs/2209.00012
http://arxiv.org/abs/2209.00012
Akademický článek
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Akademický článek
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Autor:
N Muñoz-Elgueta, F Arrigoni Battaia, G Kauffmann, C De Breuck, C García-Vergara, A Zanella, E P Farina, R Decarli
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 511(1), 1462-1483
Cool gas (T$\sim$10$^{4}$~K) traced by hydrogen Ly$\alpha$ emission is now routinely detected around $z\sim3$ quasars, but little is known about their molecular gas reservoirs. Here, we present an APEX spectroscopic survey of the CO(6-5), CO(7-6) and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f501ddb034fd461b929b034197c45438
http://arxiv.org/abs/2201.11660
http://arxiv.org/abs/2201.11660
Autor:
A. Zanella, Michael Hilker, F. Arrigoni-Battaia, Johan Richard, Francesco Valentino, Martin Zwaan, Chian-Chou Chen, Christopher Harrison, Manuel Behrendt, Eric Emsellem, Joel Vernet, Jérémy Fensch, E. Le Floc'h, Andreas Burkert, G. Rodighiero, Eros Vanzella, Pascale Hibon, Max Gronke, E. Iani, A. M. Swinbank, Vincenzo Mainieri
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 507(3), 3830-3848. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 507, pp.3830-3848. ⟨10.1093/mnras/stab2376⟩
Monthly notices of the Royal Astronomical Society, 2021, Vol.507(3), pp.3830-3848 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 507, pp.3830-3848. ⟨10.1093/mnras/stab2376⟩
Monthly notices of the Royal Astronomical Society, 2021, Vol.507(3), pp.3830-3848 [Peer Reviewed Journal]
Giant star-forming regions (clumps) are widespread features of galaxies at $z \approx 1-4$. Theory predicts that they can play a crucial role in galaxy evolution if they survive to stellar feedback for > 50 Myr. Numerical simulations show that clumps
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::51842f598cc6793076efb5ef1a45e507
https://research.rug.nl/en/publications/2dc46764-74f5-4e98-867d-932bef1c6017
https://research.rug.nl/en/publications/2dc46764-74f5-4e98-867d-932bef1c6017
Publikováno v:
Astronomy & Astrophysics, 2021, Vol.653, pp.A122 [Peer Reviewed Journal]
Contrary to expectations from scenarios of black hole growth driven by galaxy interactions and mergers, dual active galactic nuclei (AGN) with kiloparsec separations are rarely observed and are very difficult to identify, in particular at high redshi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::de2b80016c8b8dc9c1358ad2681ddc91
http://arxiv.org/abs/2107.10773
http://arxiv.org/abs/2107.10773