... DENSITY BOUNDING OF GIANT H II REGIONS AND THE IONIZATION OF THE DIFFUSE INTERSTELLAR MEDIUM . ... Three different types of evidence are presented in favour of the hypothesis that the H II regions in disc galaxies with H luminosities greater than a critical value: 10 erg s , are density bounded, and that the escaping Lyman continuum photons from these are the principal ionizing agents for the diffuse ISM in disc galaxies. ... Evidence for density bounding in the most luminous regions . ...

Next: CR Bound for Up: Cram?r-Rao Bound - Accuracy Previous: Introduction . ... The left side of (1) is the mean square error for the estimate and the right side is the bound. No estimate for a can have a mean square error smaller than the bound. From (1) we observe the following regarding changes in a : if the PDF change is large the error will be small; if, however, the PDF change is small the error is large. The CR bound estimates the sensitivity of the data to changes in a . ...

... Цвет: желтый . Коллекция: Весна-лето 2016 . ... Размер K2: 98 . ... Ветровка E-Bound. ... Цвет: серый . ... Материал верха: текстиль . ... Кеды s.Oliver. ... Коллекция: Осень-зима 2015/2016 . ... Вес велосипеда - 8, Диаметр колес - 12, Цвет - Красный, Модель - NOVATRACK Maple 12 (2015), Тип заднего тормоза - Ножной (барабанный), Область применения - Дорожный, Модельный ряд - NOVATRACK Maple (2015), Возрастная группа - Детский, Количество скоростей - 1, Модельный год - 2015, Материал рамы - Сталь . ...

... Posts tagged ?confidence bounds? ... Sometime early this year, Jeremy Drake asked this innocuous sounding question in the context of determining the bounds on the amplitude of an absorption line: Is the 3sigma error bar the same length as 3 times the 1sigma error bar? ... Likelihoodists will say ?Maybe, yeah, er, depends?, and Bayesians will say ? ... Tags: Bayesian , central limit theorem , confidence bounds , error bar , Frequentist , highest posterior density , HPD , likelihoodist , sigma . ...

Dense regions reach a maximum size and then fall back into a bound object like a cluster of galaxies. Once the cluster is formed, its physical size remains essentially constant. The space-time diagram below . shows a dense region in blue on the left. ... The galaxies in the blue region are accelerating more just because the region is denser and therefore has higher gravitational forces. ... Tutorial : Part 1 | Part 2 | ...

... Meta Index / Home Page / General-purpose array-processing utilities / Array or vector scalar . subroutine maskArrayLimits(mask, minXi, maxXi, minYi, maxYi) logical(bool), intent(in) :: mask(:,:) integer(int16), intent(out) :: minXi, maxXi, minYi, maxYi end subroutine . ... logical(bool) :: mask(4,5) mask(1,:) = ((/0, 0, 0, 0, 0/) > 0) mask(2,:) = ((/0, 1, 1, 0, 0/) > 0) mask(3,:) = ((/1, 1, 0, 1, 0/) > 0) mask(4,:) = ((/1, 0, 0, 0, 0/) > 0) call maskArrayLimits(mask, minXi, maxXi, minYi, maxYi) ! ...