2019
DOI: 10.1093/mnras/stz3148
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H i column density statistics of the cold neutral medium from absorption studies

Abstract: Physical properties of the tiny scale structures in the cold neutral medium (CNM) of galaxies is a long-standing puzzle. Only a few lines of sights in our Galaxy have been studies with mixed results on the scale-invariant properties of such structures. Moreover, since these studies measure the variation of neutral hydrogen optical depth, they do not directly constrain the density structures. In this letter, we investigate the possibility of measuring the properties of density and spin temperature structures of… Show more

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“…For estimating the unknown parameters of the Kumaraswamy distribution, the reliability function of serial and parallel systems, and the failure rate function. The estimation methods are Maximum Likelihood, Standard Bayesian and E-Bayes Methods [15], [16].…”
Section: B Estimation Methodsmentioning
confidence: 99%
“…For estimating the unknown parameters of the Kumaraswamy distribution, the reliability function of serial and parallel systems, and the failure rate function. The estimation methods are Maximum Likelihood, Standard Bayesian and E-Bayes Methods [15], [16].…”
Section: B Estimation Methodsmentioning
confidence: 99%