The exact nature of the explosion mechanism in Type I generally is still uncertain, although Ia supernovae, at least, are thought to originate in binary systems consisting of a moderately massive star and a white dwarf, with material flowing to the white dwarf from its larger companion.
The type Ia supernova, an explosion that occurs in binary systems consisting of two stars, was approximately 11.5 million light-years from Earth and is one of the closest of its type discovered in the past few decades.
The paper focuses on simulating a binary system, consisting of poorly soluble drug, dispersed in a matrix of highly soluble acid excipient.
In Part 2, we enlarge on a description of our work on Direct MC, for the particular case of simulating a binary system consisting of poorly soluble drug dispersed in a matrix of highly-soluble acid excipient.
The phase behavior and optical- and selected mechanical properties of the binary system consisting of isotactic polypropylene (i-PP) and a new sorbitol-based nucleating and clarifying agent, 1,2,3-trideoxy-4,6 5,7-bis-O-[ 4-propylphenyl) methylene]-nonitol (TBPMN), were investigated.
The phase behavior of the binary system consisting of isotactic polypropylene (i-PP) and N,N′,N″-tris-isopentyl-1,3,5-benzene-tricarboxamide (1)—a selected member of a class of novel, versatile 'designer' nucleating/clarifying agents was investigated over the entire additive concentration range by means of differential scanning calorimetry (DSC) and optical microscopy.
Also known as Nova Muscae 1983, GQ Muscae is a binary system consisting of a white dwarf and small star that is about 10% as massive as the Sun.
The progenitor binary system consists of main sequence stars, with the primary possessing more mass than the secondary.
In the developing regime, the derivation is based on that of a pseudo-binary system, consisting of one of the feed components and the sweep gas.
