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Because of the high number of field [[stars]] from the [[Milky_Way#Composition_and_structure|disc of the Milky Way]], i ...the [[Sun]], its mean [[Extinction (astronomy)|visual extinction]] <math>E(B-V) = 0.27</math> and its age to range from <math>6\times 10^{7}</math> and ...

...tar]]'s orbital plane, induced by gravitational perturbations from passing stars. ...and that is embedded in a [[stellar system]] containing a large number of stars. Let <math>M_1</math> and <math>M_2</math> be the masses of the two compon ...

:<math> \frac{15}{4\pi^4}\int_0^x \frac{t^7e^{2t}}{(e^t-1)^3} \, dt .</math> ...r absorption coefficients and opacities|title= Stellar Structure |series= Stars and Stellar Systems: Compendium of Astronomy and Astrophysics |volume=VIII| ...

...e at ESO’s [[La Silla Observatory]] in Chile.<ref>{{cite web|title=Sibling Stars|url=http://www.eso.org/public/news/eso1534/|access-date=19 August 2015}}</r ...drogen]] and [[helium]].<ref name=aaa424/> The combined mass of the active stars in this cluster is about 630 times the [[mass of the Sun]].<ref name=aaa386 ...

...l |bibcode=2018MNRAS.480.3706K |title=On the evolutionary state of massive stars in transition phases in M33 |last1=Kourniotis |first1=M. |last2=Kraus |firs | luminosity = {{val|4.68|e=6}} ...

|b-v= |u-b= ...

...=The wind speeds, dust content, and mass-loss rates of evolved AGB and RSG stars at varying metallicity|year=2016|journal=[[Monthly Notices of the Royal Ast ...name=":0">{{Cite journal|last1=Matsuura|first1=Mikako|last2=Sargent|first2=B.|last3=Swinyard|first3=Bruce|last4=Yates|first4=Jeremy|last5=Royer|first5=P ...

...assband|pass bands]] (U, B, and V), although often, an average of multiple stars is used for higher accuracy.<ref name=":0">{{Cite book |title=Introduction ...taine|first7=N.|last8=Christensen-Dalsgaard|first8=J.|last9=Depagne|first9=E.|date=2015-10-21|title=IAU 2015 Resolution B2 on Recommended Zero Points fo ...

| b-v=+2.10<ref name=klare/> | u-b=+0.75<ref name=klare/> ...

...ry/optical-IR-prod/wds/orb6|title=Sixth Catalog of Orbits of Visual Binary Stars|work=United States Naval Observatory|access-date=2017-03-11|archive-date=20 | b-v = ...

...els obeying [[Jaffe's law]] in the density. The isotropic model, <math>f=f(E)</math>, is plotted with the heavy line.]] ...(representing stars) in a specified gravitational potential (in which the stars move). The density and potential need not be self-consistently related. ...

...ts significantly different from the stellar disk. This includes metal-poor stars (with low [Fe/H] < -1), which likely belong to the [[stellar halo]] or [[Ac ...first=George|date=1962|title=Abundances in G Dwarfs. VI. A Survey of Field Stars |journal=The Astrophysical Journal Supplement Series|language=en|volume=6|p ...

| b-v = +1.61<ref name=Mermilliod1986/> | u-b = +1.96<ref name=Mermilliod1986/> ...

| b-v = {{Val|+2.419|0.014}}<ref name=Anderson2012/> | u-b = +2.93<ref name=UBV/> ...

| u-b = −0.50<ref name=Johnson1966/> | b-v = −0.14<ref name=Johnson1966/> ...

| b-v=0.84<ref name=ducati/> | u-b=-0.19<ref name=ducati/> ...

...-Enceladus galaxy. Yellow arrows represent the positions and velocities of stars originating from the dwarf galaxy, the data taken from a simulated merger w | mass = {{Val|5|e=10}} ...

| b-v = +1.21<ref name = Mermilliod1986/> | u-b = +1.25<ref name = Mermilliod1986/> ...

{{about|p² Leonis|other stars with this Bayer designation|p Leonis}} | b-v = {{Val|+1.593|0.059}}<ref name=Anderson2012/> ...

| b-v = 0.49<ref name="Borgniet2017"/> ...n the case of 38 Virginis, only one was discovered, which was designated ''b''.<ref name="Borgniet2017"/> ...