Super Soft Peach-Phase(SSP).

Super Soft Sources

Super Soft Sources (SSS) are characterized by radiation with effective temperatures of ∼10 to ∼10 K and luminosities of ∼10 to ∼10 erg s. The first luminous SSS in the Large Magellanic Cloud (LMC) have been discovered around 1980 with the Einstein observatory (Long et al. 1981). Optical identifications for both CAL 83 and CAL 87 established the binary nature of these sources (Cowley et al. 1990...

Phony Peach and Peach Mosaic

Slow-moving and far-travelled dense pyroclastic flows during the Peach Spring super-eruption

Explosive volcanic super-eruptions of several hundred cubic kilometres or more generate long run-out pyroclastic density currents the dynamics of which are poorly understood and controversial. Deposits of one such event in the southwestern USA, the 18.8 Ma Peach Spring Tuff, were formed by pyroclastic flows that travelled >170 km from the eruptive centre and entrained blocks up to ∼ 70-90 cm di...

Super-resolution Target Mapping from Soft-Classified Remotely Sensed Imagery

A simple, efficient algorithm is presented for super-resolution target mapping from remotely sensed images. Following an initial random allocation of pixel proportions to binary 'hard' sub-pixel classes, the algorithm works in a series of iterations, each of which contains two stages. For each iteration, a distance weighted function of neighbouring pixels is computed for all sub-pixels. Then, o...

Soft nuclear equations of state for super-massive neutron star

Two new nuclear equations of state (EOSs) are proposed and are applied to neutron star (NS). They predict the incompressibilitiesK0 = 179MeV and 230MeV, respectively. The density dependencies of nuclear symmetry energies are consistent with the recent analyses of heavy-ion reactions. We can reproduce the recently observed super-massive NS of MG > 2:5M , the mass-radius relation of EXO 0748-676 ...