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PV Telescopii is a class B-type (blue) extreme helium star that is the prototype of a class of variables known as PV Telescopii variables.
We then computed multivariate models within a class of variables.
We began with univariate regressions within a class of variables (i.e., demographic, patient-reported outcome, clinical-chart nodes).
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Some binaries form a class of variable stars (see eclipsing variable star).
For 100 years astronomers have paid particular attention to a class of variable star known as the Cepheids.
Another prominent variable star is RR Lyrae, which gave its name to a class of variable stars that are used in measuring distances to other galaxies.
Algol, also called Beta Persei, prototype of a class of variable stars called eclipsing binaries, the second brightest star in the northern constellation Perseus.
Cepheid variable, one of a class of variable stars whose periods (i.e., the time for one cycle) of variation are closely related to their luminosity and that are therefore useful in measuring interstellar and intergalactic distances.
This algorithm was employed for solving a class of variable-order fractional differential equations.
Therefore, it is the aim of this paper to derive a class of variable-coefficient tempered fractional diffusion models.
In this paper, the Crank-Nicolson method is proposed for solving a class of variable-coefficient tempered-FDEs (1).
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