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Disambiguation of "Lagos, P."

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The MUSE 3D view of feedback in a high-metallicity radio galaxy at z = 2.9

, , , , , , , , , , and . (2017)cite arxiv:1711.10601Comment: 25 pages, 18 figures, 10 tables. Accepted for publication in MNRAS. Published: 23 November 2017.
DOI: 10.1093/mnras/stx3019

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Flavio Lagos Galván

Soledad Lagos Kassai

Mariana Lagos-Quintana

Markus Lagos

Sonia Lagos-Witte

 

Other publications of authors with the same name

On the properties of the interstellar medium in extremely metal-poor blue compact dwarf galaxies: GMOS-IFU spectroscopy and SDSS photometry of the double-knot galaxy HS 2236+1344, , , , , and . (2014)cite arxiv:1405.7070Comment: 15 pages, 16 figures, accepted for publication in A&A.The MUSE 3D view of feedback in a high-metallicity radio galaxy at z = 2.9, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1711.10601Comment: 25 pages, 18 figures, 10 tables. Accepted for publication in MNRAS. Published: 23 November 2017.Ionization and feedback in Ly$\alpha$ halos around two radio galaxies at z$\sim$2.5, , , , , , , , and . (2016)cite arxiv:1611.05739.An accurate low-redshift measurement of the cosmic neutral hydrogen density, , , , , , , , , and . (2019)cite arxiv:1907.10375Comment: 17 pages, 24 figures.On the evolution of the molecular gas fraction of star forming galaxies, , , , , and . (2011)cite arxiv:1102.3694 Comment: Accepted for publication in ApJ Letters; 5 pages, 2 figures.The HI mass function as a probe of photoionisation feedback on low mass galaxy formation, , , , , and . (2015)cite arxiv:1506.02736Comment: 12 pages, 9 figures, Submitted to MNRAS.Predictions for the CO emission of galaxies from a coupled simulation of galaxy formation and photon dominated regions, , , , , , and . (2012)cite arxiv:1204.0795Comment: 23 pages, 13 figures. Submitted to MNRAS.The initial mass function and star formation law in the outer disc of NGC 2915, , , , , , and . (2014)cite arxiv:1411.6674Comment: 19 pages, 15 figures, accepted for publication in MNRAS on 20 November 2014.The cosmic radio background from 150 MHz--8.4 GHz, and its division into AGN and star-forming galaxy flux, , , , , , and . (2023)cite arxiv:2301.03699.It's not easy being green: The evolution of galaxy colour in the EAGLE simulation, , , , , , and . (2016)cite arxiv:1601.07907Comment: 15 pages, 10 figures. Submitted to MNRAS. All comments welcome. Larger version of Fig. 1 included in source. For the animated evolution of the EAGLE intrinsic u-r CMD (with central and satellite galaxies coloured red and blue respectively) see http://community.dur.ac.uk/j.w.trayford/media/CMD_evolution_EAGLE.mp4.