On the viability of determining galaxy properties from observations I: Star formation rates and kinematics
| Autor: | Kearn Grisdale, Laurence Hogan, Dimitra Rigopoulou, Niranjan Thatte, Miguel Pereira-Santaella, Julien Devriendt, Adrianne Slyz, Ismael García-Bernete, Yohan Dubois, Sukyoung K Yi, Katarina Kraljic |
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| Přispěvatelé: | Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS) |
| Jazyk: | angličtina |
| Rok vydání: | 2022 |
| Předmět: |
FOS: Physical sciences
Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics - Astrophysics of Galaxies galaxies: high-redshift [SDU]Sciences of the Universe [physics] Space and Planetary Science cosmology: observations Astrophysics of Galaxies (astro-ph.GA) galaxies: structure Astrophysics - Instrumentation and Methods for Astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) galaxies: kinematics and dynamics Astrophysics::Galaxy Astrophysics |
| Zdroj: | Monthly Notices of the Royal Astronomical Society Monthly Notices of the Royal Astronomical Society, 2022, ⟨10.1093/mnras/stac1124⟩ |
| ISSN: | 0035-8711 1365-2966 |
| Popis: | We explore how observations relate to the physical properties of the emitting galaxies by post-processing a pair of merging $z\sim2$ galaxies from the cosmological, hydrodynamical simulation NewHorizon using LCARS (Light from Cloudy Added to RAMSES) to encode the physical properties of the simulated galaxy into H$\alpha$ emission line. By carrying out mock observations and analysis on these data cubes we ascertain which physical properties of the galaxy will be recoverable with the HARMONI spectrograph on the European Extremely Large Telescope (ELT). We are able to estimate the galaxy's star formation rate and dynamical mass to a reasonable degree of accuracy, with values within a factor of $1.81$ and $1.38$ of the true value. The kinematic structure of the galaxy is also recovered in mock observations. Furthermore, we are able to recover radial profiles of the velocity dispersion and are therefore able to calculate how the dynamical ratio varies as a function of distance from the galaxy centre. Finally, we show that when calculated on galaxy scales the dynamical ratio does not always provide a reliable measure of a galaxy's stability against gravity or act as an indicator of a minor merger. Comment: 20 pages, 17 figures, Accepted for Publication in MNRAS, Comments and questions welcome |
| Databáze: | OpenAIRE |
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