Exploring the "--" relation of HII galaxies and giant extragalactic HII regions acting as standard candles
arXiv:1911.10959 · doi:10.3847/1538-4357/ab5b94
Abstract
Cosmological applications of HII galaxies (HIIGx) and giant extragalactic HII regions (GEHR) to construct the Hubble diagram at higher redshifts require knowledge of the "--" relation of the standard candles used. In this paper, we study the properties of a large sample of 156 sources (25 high- HII galaxies, 107 local HII galaxies, and 24 giant extragalactic HII regions) compiled by Terlevich et al.(2015). Using the the cosmological distances reconstructed through two new cosmology-independent methods, we investigate the correlation between the H emission-line luminosity and ionized-gas velocity dispersion . The method is based on non-parametric reconstruction using the measurements of Hubble parameters from cosmic clocks, as well as the simulated data of gravitational waves from the third-generation gravitational wave detector (the Einstein Telescope, ET), which can be considered as standard sirens. Assuming the emission-line luminosity versus ionized gas velocity dispersion relation, HH, we find the full sample provides a tight constraint on the correlation parameters. However, similar analysis done on three different sub-samples seems to support the scheme of treating HII galaxies and giant extragalactic HII regions with distinct strategies. Using the corrected "--" relation for the HII observational sample beyond the current reach of Type Ia supernovae, we obtain a value of the matter density parameter, (calibrated with standard clocks) and (calibrated with standard sirens), in the spatially flat CDM cosmology.
9 pages, 5 figures, 1 table, accepted for publication in ApJ
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