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

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 toward their centers, induce intense bursts of star f...

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Detalles Bibliográficos
Autores principales: 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.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2022
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9355969/
https://www.ncbi.nlm.nih.gov/pubmed/35931777
http://dx.doi.org/10.1038/s41467-022-32297-x

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9355969/
https://www.ncbi.nlm.nih.gov/pubmed/35931777
http://dx.doi.org/10.1038/s41467-022-32297-x

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