Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star-forming Galaxies at z < 3

Autor: Axel Wei ß, Christopher C. Hayward, Manuel Aravena, Sreevani Jarugula, Paul van der Werf, Matthieu Béthermin, Chenxing Dong, Yordanka Apostolovski, A. C. Mangian, Cassie Reuter, Kedar A. Phadke, Joaquin Vieira, Desika Narayanan, Yashar D. Hezaveh, Chian-Chou Chen, Carlos De Breuck, D. J. M. Cunningham, Thomas R. Greve, Justin Spilker, Katrina C. Litke

Publikováno v: Astrophysical Journal (0004-637X), 880(2), 92
The Astrophysical Journal
The Astrophysical Journal, 2019, 880, ⟨10.3847/1538-4357/ab290d⟩
Jarugula, S, Vieira, J D, Spilker, J S, Apostolovski, Y, Aravena, M, Bethermin, M, de Breuck, C, Chen, C-C, Cunningham, D J M, Dong, C, Greve, T, Hayward, C C, Hezaveh, Y, Litke, K C, Mangian, A C, Narayanan, D, Phadke, K, Reuter, C A, Van der Werf, P & Weiss, A 2019, ' Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star-forming Galaxies at z ∼ 3 ', Astrophysical Journal Supplement Series, vol. 880, no. 2, 92 . https://doi.org/10.3847/1538-4357/ab290d

International audience; Water (H2O), one of the most ubiquitous molecules in the universe, has bright millimeter-wave emission lines that are easily observed at high redshift with the current generation of instruments. The low-excitation transition o

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d05fa5a15114261d98fe7ee8c45221c3
http://hdl.handle.net/1887/84211