Sentence examples for emitting region from inspiring English sources

Analysis shows that (36 ± 6)% of the excitons form in the blue emitting region, while (64 ± 6)% form in the green emitting region at 100 mA/cm2.

We briefly show analysis and results of the height of hard X-ray emitting region.

We derive constraints on the line emitting region from the relative strength of the CaII triplet, OI λ8446 and Hβ.

We modeled the continuum and line emitting region and simulate a lensing event by a star cluster located in an intervening galaxy.

Proposed explanations include a reduced X-ray emitting region (a heated polar cap), or the presence of a bare quark/strange star.

First, I will present how we can constrain the physical conditions of the GRB emitting region by using indirect information from the copious neutrino emission that is naturally produced via photohadronic interactions on an ad-hoc Band photon spectrum.

The emergent portions of such helically deformed, undulating flux tube show a series of S-shaped X-ray emitting regions as observed by the Yohkoh satellite.

Using the primary result of our analisys — that the observed emission is of synchrotron origin — we derive information on the physical parameters of GRB emitting regions.

The HETGS allows one to probe the physical parameters of emitting regions of all classes of X-ray sources, including stars, X-ray binaries, supernova remnants, galaxies, clusters of galaxies, quasars, and interstellar and intergalactic material.

Using the resonance, intercombination and forbidden lines of the few prominent helium-like ions, we infer a density greater than 2 × 1012 cm−3 and a temperature of ∼2 MK for the oxygen and neon line emitting regions in the accretion column of AM Her.

Hence, our estimate of the magnetic field strength in the range of 12 128 mG represents a lower-limit for the NIR emitting regions of the torus of IC5063.