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Molecular gas content and high excitation of a massive main-sequence galaxy at z = 3

Autor: Lei, Han, Valentino, Francesco, Magdis, Georgios E., Kokorev, Vasily, Liu, Daizhong, Rigopoulou, Dimitra, Jin, Shuowen, Daddi, Emanuele

Publikováno v: Lei, H, Valentino, F, Magdis, G E, Kokorev, V, Liu, D, Rigopoulou, D, Jin, S & Daddi, E 2023, ' Molecular gas content and high excitation of a massive main-sequence galaxy at z = 3 ', Astronomy & Astrophysics, vol. 673, L13 . https://doi.org/10.1051/0004-6361/202345925
Lei, H, Valentino, F, Magdis, G E, Kokorev, V, Liu, D, Rigopoulou, D, Jin, S & Daddi, E 2023, ' Molecular gas content and high excitation of a massive main-sequence galaxy at z = 3 ', Astronomy and Astrophysics, vol. 673, L13 . https://doi.org/10.1051/0004-6361/202345925

We present new CO ($J=5-4$ and $7-6$) and [CI] ($^3P_2\,-\, ^3P_1$ and $^3P_1\,-\, ^3P_0$) emission line observations of the star-forming galaxy D49 at the massive end of the Main Sequence at $z=3$. We incorporate previous CO ($J=3-2$) and optical-to

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8461f737097630cf9ded6c29a2e3466b
https://curis.ku.dk/portal/da/publications/molecular-gas-content-and-high-excitation-of-a-massive-mainsequence-galaxy-at-z--3(43da2655-d646-4862-9614-874e745d0ad9).html

Exploring the environment, magnetic fields, and feedback effects of massive high-redshift galaxies with [CII]

Autor: K. Kade, K. K. Knudsen, W. Vlemmings, F. Stanley, B. Gullberg, S. König

Publikováno v: Kade, K, Knudsen, K K, Vlemmings, W, Stanley, F, Gullberg, B & König, S 2023, ' Exploring the environment, magnetic fields, and feedback effects of massive high-redshift galaxies with [CII] ', Astronomy and Astrophysics, vol. 673, A116 . https://doi.org/10.1051/0004-6361/202141839

Context. Massive galaxies are expected to grow through different transformative evolutionary phases. High-redshift starburst galaxies and quasars are thought to be such phases and thus provide insight into galaxy evolution. Several physical mechanism

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a6ad354eadcb909c0d97cb194202eb51
http://arxiv.org/abs/2305.03812

A solar metallicity galaxy at z > 7? Possible detection of the [N II] 122 mu m and [O III] 52 mu m lines

Autor: Meghana Killi, Darach Watson, Seiji Fujimoto, Hollis Akins, Kirsten Knudsen, Johan Richard, Yuichi Harikane, Dimitra Rigopoulou, Francesca Rizzo, Michele Ginolfi, Gergö Popping, Vasily Kokorev

Publikováno v: Killi, M, Watson, D, Fujimoto, S, Akins, H, Knudsen, K, Richard, J, Harikane, Y, Rigopoulou, D, Rizzo, F, Ginolfi, M, Popping, G & Kokorev, V 2023, ' A solar metallicity galaxy at z > 7? Possible detection of the [N II] 122 mu m and [O III] 52 mu m lines ', Monthly Notices of the Royal Astronomical Society, vol. 521, no. 2, pp. 2526-2534 . https://doi.org/10.1093/mnras/stad687

We present the first detection of the [N II] 122 $\mu$m and [O III] 52 $\mu$m lines for a reionisation-epoch galaxy. Based on these lines and previous [C II] 158 $\mu$m and [O III] 88 $\mu$m measurements, using two different radiative transfer models

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8dcecd69935dbc5deb97bcca0dc3e871
https://curis.ku.dk/ws/files/345315204/stad687.pdf

WISDOM Project – X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure

Autor: Timothy A Davis, Jindra Gensior, Martin Bureau, Michele Cappellari, Woorak Choi, Jacob S Elford, J M Diederik Kruijssen, Federico Lelli, Fu-Heng Liang, Lijie Liu, Ilaria Ruffa, Toshiki Saito, Marc Sarzi, Andreas Schruba, Thomas G Williams

Publikováno v: Davis, T A, Gensior, J, Bureau, M, Cappellari, M, Choi, W, Elford, J S, Kruijssen, J M D, Lelli, F, Liang, F-H, Liu, L, Ruffa, I, Saito, T, Sarzi, M, Schruba, A & Williams, T G 2022, ' WISDOM Project-X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure ', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 1, pp. 1522-1540 . https://doi.org/10.1093/mnras/stac600
Davis, T A, Gensior, J, Bureau, M, Cappellari, M, Choi, W, Elford, J S, Kruijssen, J M D, Lelli, F, Liang, F-H, Liu, L, Ruffa, I, Saito, T, Sarzi, M, Schruba, A & Williams, T G 2022, ' WISDOM Project-X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure ', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 1, pp. 1522–1540 . https://doi.org/10.1093/mnras/stac600

We use high-resolution maps of the molecular interstellar medium (ISM) in the centres of eighty-six nearby galaxies from the millimetre-Wave Interferometric Survey of Dark Object Masses (WISDOM) and Physics at High Angular Resolution in Nearby Galaxi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fc0eb9d8eb29c845411e80da31e0d822
https://doi.org/10.1093/mnras/stac600