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Unveiling the warm and dense ISM in z > 6 quasar host galaxies via water vapor emission

Autor: A. Pensabene, P. van der Werf, R. Decarli, E. Bañados, R. A. Meyer, D. Riechers, B. Venemans, F. Walter, A. Weiß, M. Brusa, X. Fan, F. Wang, J. Yang

Publikováno v: Astronomy & Astrophysics, 667:A9

Water vapor (H$_{2}$O) is one of the brightest molecular emitters after carbon monoxide (CO) in galaxies with high infrared (IR) luminosity, and allows us to investigate the warm dense phase of the interstellar medium (ISM) where star formation occur

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3eca7ff4fc1b193e1dd656dcb67238bb
https://hdl.handle.net/1887/3514990

The ALMA REBELS Survey: cosmic dust temperature evolution out to z~7

Autor: L Sommovigo, A Ferrara, A Pallottini, P Dayal, R J Bouwens, R Smit, E da Cunha, I De Looze, R A A Bowler, J Hodge, H Inami, P Oesch, R Endsley, V Gonzalez, S Schouws, D Stark, M Stefanon, M Aravena, L Graziani, D Riechers, R Schneider, P van der Werf, H Algera, L Barrufet, Y Fudamoto, A P S Hygate, I Labbé, Y Li, T Nanayakkara, M Topping

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 513(3), 3122-3135
Sommovigo, L, Ferrara, A, Pallottini, A, Dayal, P, Bouwens, R J, Smit, R, Da cunha, E, De looze, I, Bowler, R A A, Hodge, J, Inami, H, Oesch, P, Endsley, R, Gonzalez, V, Schouws, S, Stark, D, Stefanon, M, Aravena, M, Graziani, L, Riechers, D, Schneider, R, Van der werf, P, Algera, H, Barrufet, L, Fudamoto, Y, Hygate, A P S, Labbé, I, Li, Y, Nanayakkara, T & Topping, M 2022, ' The ALMA REBELS Survey : cosmic dust temperature evolution out to z ∼ 7 ', Monthly Notices of the Royal Astronomical Society, vol. 513, no. 3, pp. 3122-3135 . https://doi.org/10.1093/mnras/stac302
Monthly Notices of the Royal Astronomical Society, 513(3), 3122-3135. Oxford University Press
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

ALMA observations have revealed the presence of dust in the first generations of galaxies in the Universe. However, the dust temperature Td remains mostly unconstrained due to the few available FIR continuum data at redshift $z$ > 5. This introduces

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::339c1b75ed0983ce3f39e506dfd29829

PRUSSIC

Autor: M. Rybak, J. A. Hodge, T. R. Greve, D. Riechers, I. Lamperti, J. van Marrewijk, F. Walter, J. Wagg, P. P. van der Werf

Publikováno v: Rybak, M, Hodge, J A, Greve, T R, Riechers, D, Lamperti, I, van Marrewijk, J, Walter, F, Wagg, J & van der Werf, P P 2022, ' I. A JVLA survey of HCN, HCO +, and HNC (1–0) emission in z ∼ 3 dusty galaxies: Low dense-gas fractions in high-redshift star-forming galaxies ⋆ ', Astronomy and Astrophysics, vol. 667, A70 . https://doi.org/10.1051/0004-6361/202243894
Astronomy & Astrophysics, 667

Dusty star-forming galaxies (DSFGs) at redshift z$\geq$1 are among the most vigorously star-forming galaxies in the Universe. However, their dense ($\geq$10$^5$ cm$^{-3}$ ) gas phase - typically traced by HCN(1-0) - remains almost entirely unexplored

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ad066786f1a758e23e669b7f5cb8568
https://doi.org/10.1051/0004-6361/202243894