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<ref name="proxima b discovery paper">{{cite journal | bibcode = 2016Natur.536..437A | title = A terrestrial planet candidate in a temperate orbit around Proxima Centauri | journal = Nature | volume = 536 | issue = 7617 | pages = 437–440 | last1 = Anglada-Escudé | first1 = Guillem | last2 = Amado | first2 = Pedro J. | last3 = Barnes | first3 = John | last4 = Berdiñas | first4 |
Citation bot (talk | contribs) Alter: doi-broken-date. | Use this bot. Report bugs. | Suggested by AManWithNoPlan | #UCB_webform 438/2165 |
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:<math>\frac{M_{2}^{3}}{M_\mathrm{tot}^{2}} = \frac{\omega_\mathrm{orb}^{2} a_{1}^{3}}{G}.</math>
The peak radial velocity of object 1, <math>K</math>, depends on the orbital inclination <math>i</math> (an inclination of 0° corresponds to an orbit seen face-on, an inclination of 90° corresponds to an orbit seen edge-on). For a circular orbit ([[orbital eccentricity]] = 0) it is given by<ref name="tauris">{{cite book |last1=Tauris |first1=T.M. |last2=van den Heuvel |first2=E.P.J. |author2-link=Ed van den Heuvel |editor1-last=Lewin |editor1-first=Walter |editor1-link=Walter Lewin |editor2-last=van der Klis |editor2-first=Michiel |editor2-link=Michiel van der Klis |title=Compact stellar X-ray sources |url=https://archive.org/details/compactstellarxr00whgl |url-access=limited |publisher=Cambridge, UK: [[Cambridge University Press]] |date=2006 |pages=[https://archive.org/details/compactstellarxr00whgl/page/n640 623]–665 |chapter=Chapter 16: Formation and evolution of compact stellar X-ray sources |arxiv=astro-ph/0303456 |isbn=978-0-521-82659-4 |doi=10.2277/0521826594 |name-list-style=amp|doi-broken-date=31
:<math>K = v_{1} \mathrm{sin} i = \omega_\mathrm{orb} a_{1} \mathrm{sin} i.</math>
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