Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913

Autor: Ginolfi, M, Piconcelli, E, Zappacosta, L, Jones, GC, Pentericci, L, Maiolino, R, Travascio, A, Menci, N, Carniani, S, Rizzo, F, Arrigoni Battaia, F, Cantalupo, S, De Breuck, C, Graziani, L, Knudsen, K, Laursen, P, Mainieri, V, Schneider, R, Stanley, F, Valiante, R, Verhamme, A

Publikováno v: Ginolfi, M, Piconcelli, E, Zappacosta, L, Jones, G C, Pentericci, L, Maiolino, R, Travascio, A, Menci, N, Carniani, S, Rizzo, F, Arrigoni Battaia, F, Cantalupo, S, De Breuck, C, Graziani, L, Knudsen, K, Laursen, P, Mainieri, V, Schneider, R, Stanley, F, Valiante, R & Verhamme, A 2022, ' Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913 ', Nature Communications, vol. 13, no. 1, 4574 . https://doi.org/10.1038/s41467-022-32297-x

The phase transition between galaxies and quasars is often identified with the rare population of hyper-luminous, hot dust-obscured galaxies. Galaxy formation models predict these systems to grow via mergers, that can deliver large amounts of gas tow

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b99c41a2705540dd56f08eb6730db1c
http://arxiv.org/abs/2208.03248