Two of these turned out to be hot emission-line stars, of which one is a definite B[e] star. The mass-loss rates were measured through modelling of the spectral energy distributions. We thus obtain the massloss rate formula log. M = - 5.65 + 1.05 log(L/10 000 L-circle dot) - ...
Gravitational-wave emission from binary black holes formed in open clusters. Mon. Not. R. Astron. Soc. 2019, 486, 3942–3950. [Google Scholar] [CrossRef] Kumamoto, J.; Fujii, M.S.; Tanikawa, A. Merger rate density of binary black holes formed in open clusters. arXiv 2020, arXiv:...
If one considers the absorption (emission) of electromagnetic radiation by atoms, the probability of the occurrence of a transition between two unperturbed states ψi and ψf as caused by the interaction of an electromagnetic radiation field and a crystal is dependent on the matrix element (1)∫...
Kumamoto J, Fujii MS, Tanikawa A (2019) Gravitational-wave emission from binary black holes formed in open clusters. MNRAS 486(3):3942–3950 Article ADS Google Scholar Kumamoto J, Fujii MS, Tanikawa A (2020) Merger rate density of binary black holes formed in open clusters. MNRAS 495(4...
The imaging was performed using DAPI (excitation 335–383 nm; emission 420–470 nm) dichroic filter cubes. The images were acquired in mosaic mode with a ×10 objective and 10% tile overlap. The resulting tiles were stitched together before being exported in TIFF file format using ZEN ...
(Fig.1). This line defines the limit beyond which the nuclei are unbound with respect to proton emission4. Thus, to unveil the mechanisms of the rp process, the properties of very exotic neutron-deficient nuclei need to be known. However, the relevant nuclei are typically characterized by ...
All elements with an atomic number (Z) greater than 83, and/or atomic mass (A) greater than 209 are radioactive—that is, they decay sponta neously into other elements, and this decay causes the emission of active particles. To specifically designate each individual atom, certain symbols ...
To calculate the Fractional Synthesis Rate (FSR) we used the formula previously utilized33: $${\text{FSR }} = {\text{ sAPP Slope }} \div {\text{ Precursor E}}$$ sAPP Slope is the slope of the linear regression from 7 to 20 h for either sAPPβ or sAPPα. Precursor E is the ...
Effects on the Sunyaev–Zel'dovich effect and the X‐ray emission We performed high-resolution simulations of a sample of 14 galaxy clusters that span a mass range from 5 10 13 to 2 10 15 h 1 M to study t... C Pfrommer,T. A. Enlin,V Springel,... - 《Monthly Notices of the...
2.7. Water-related electricity use and GHG emission analysis Similar to the boundary selection for the water system performance analysis, the system boundary for the energy and GHG emissions analysis is set at the administrative boundary of Cape Town. Data are collected from water infrastructure opera...