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{{Short description|Mira-type long period variable star in the constellation Corona Borealis}} '''V Coronae Borealis''' ('''V CrB''') is a [[Mira variable|Mira-type]] long period [[variable star]] and [[carbon star]] in the [[constella ...

...inis is classified as a [[carbon star]]. SS Virginis, like all carbon Mira variables, has a [[hydrogen-alpha]] emission line that varies widely, synchronized wi [[Category:Mira variables]] ...

| variable = [[Mira variable|Mira]]<ref name = Samus2017/> ...4/> Observations from 1955 to 1967 revealed that the star was a probable [[Mira variable]]<ref name = Feuchter1967/> and was given its current designation. ...

| variable=[[Mira variable|Mira]]<ref name=gcvs/> '''R Fornacis''' is a [[Mira variable]] and [[carbon star]] located in the constellation [[Fornax]]. It ...

| variable = [[Mira variable|Mira]]<ref name=gcvs/> '''LL Pegasi''' ('''AFGL 3068''') is a [[Mira variable]] star surrounded by a pinwheel-shaped nebula, '''IRAS 23166+1655' ...

|variable = [[Mira variable|Mira]]?<ref name=gcvs/> ...below 17.8. It was classified as a long-period variable, now known as a [[Mira variable]], on the basis of its large amplitude and reasonably regular ligh ...

* <math>x_{nt}</math> are [[State variable|state variables]], with <math>x_{n0}</math> the agent's [[initial condition]] ...constraints imposed by the model, and expressed in terms of the additional variables that describe the model's structure. This approach requires powerful optimi ...

...rence between the mean and the median.<ref name=Mira1999>[[Antonietta Mira|Mira A]] (1999) "Distribution-free test for symmetry based on Bonferroni’s measu ...e limiting behaviour of the mode and median of a sum of independent random variables". ''Annals of Probability'' 8: 419–430</ref> ...

In 2013 the luminosity of Mira variables, based on [[Hipparcos]] parallaxes, was used to calibrate a [[Period-lumino ...

...ensing Experiment. The OGLE-III Catalog of Variable Stars. IV. Long-Period Variables in the Large Magellanic Cloud|journal=Acta Astronomica|volume=59|issue=3|pa ...Luminosity and Period-Luminosity-Color Relations at Maximum Light for Mira Variables in the Magellanic Clouds |last1=Bhardwaj |first1=Anupam |last2=Kanbur |firs ...

...n between the periods and the brightness of a sample of 25 of the Cepheids variables in the Small Magellanic Cloud, published in 1912.<ref name="Leavitt1912">{{ ...wing that there is a simple relation between the brightness of the Cepheid variables and their periods.<ref name="Leavitt1912"/>}} Using the simplifying assump ...

...f a set of <math>n</math> nodes and a collection of [[Social network|tie]] variables <math>\{ Y_{ij}: i=1,\dots,n; j=1,\dots,n\}</math>, indexed by pairs of nod ...ay, it is possible to describe any kind of dependence between the undyadic variables: ...

| Equation Doppler<ref>Doppler uses other symbols for the variables than we usually do today: f = 1/n, f ' = 1/x, v_o = α_o * Fluctuations in the period of variable stars like [[Mira]] (according to Doppler its period varies between 328 and 335 days), result ...

..., fluid flow or information flow. Basically, they are models whose [[state variables]] tend to be [[non-negative]] (such as mass, concentrations, energy). So th ...the axosomatodendritic axis of neurons using compartmental models]. In J. Mira & J. R. Alvarez (Eds.), Computational Methods in Neural Modeling, Pt 1 (Vol ...