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This is a single-lined [[spectroscopic binary]] star system with an [[orbital period]] of 258.48 days and an | title=An abundance analysis of the single-lined spectroscopic binaries with barium stars-like orbital elements. I. Analysis and results ...

| title=Hipparcos Photocentric Orbits of 72 Single-lined Spectroscopic Binaries This is a single-lined [[spectroscopic binary]] system with an [[orbital period]] of 2.8 years and an [[orbit ...

φ Cygni is a double-lined [[spectroscopic binary]] system, which means that the [[absorption line]]s of both componen ...rnal|bibcode=2000A&AS..145..215P|title=Resolved double-lined spectroscopic binaries: A neglected source of hypothesis-free parallaxes and stellar masses|journa ...

'''6 Draconis''' is a single-lined [[spectroscopic binary]]<ref name=Griffin1990/> [[star]] system in the northern [[constella | title= The spectroscopic orbit of 6 Draconis ...

...atic Search for Members of the Hyades Supercluster - Part Two - the Visual Binaries | last1=Eggen | first1=O. J. | journal=Astronomical Journal | volume=89:6 | This is a [[spectroscopic binary]]—orbital motion from the two stars can be detected by [[Doppler shi ...

| title=Statistical Constraints for Astrometric Binaries with Nonlinear Motion | title=High-resolution spectroscopic survey of 671 GK giants ...

Hydrogen-deficient donor stars in W Ser-esque binaries, such as the primary in HD 326823, will likely explode in Type Ib/c superno [[Category:Spectroscopic binaries]] ...

...[[Beta Lyrae variable|β Lyr]]<ref name="stickland">{{cite journal | title=Spectroscopic binary orbits from ultraviolet radial velocities. Paper 15: LY Aurigae (HD ...te journal|bibcode= 2004A&A...424..727P|title= SB9: The ninth catalogue of spectroscopic binary orbits|journal= Astronomy and Astrophysics|volume= 424|issue= 2|page ...

...erefore young, private communication indicated that Kappa Fornacis was a [[spectroscopic binary]], leaving the possibility that a companion star was the source of t ...o approximately equal-mass red dwarfs orbiting each other every ~3.7 days. Binaries with such close orbits typically maintain high levels of activity for their ...

This system is what astronomers term a double-lined [[spectroscopic binary]]. When the [[spectrum]] is examined, the [[absorption line]] featur ...ng | first4=J. H. | last5=Aerts | first5=C. | title=The orbit of the close spectroscopic binary epsilon Lup and the intrinsic variability of its early B-type compon ...

Omega Eridani was long thought to be a is a single-lined [[spectroscopic binary]] system, with an [[orbital period]] of 3,057&nbsp;days (8.4 years) | title=Tidal Effects in Binaries of Various Periods ...

...unseen component (typically a [[star]] or [[exoplanet]]) in a single-lined spectroscopic [[binary star]] or in a [[planetary system]]. It can be calculated from [[O ...e="podsiadlowski">{{cite web |url=http://www-astro.physics.ox.ac.uk/~podsi/binaries.pdf |title=The Evolution of Binary Systems, in Accretion Processes in Astro ...

HD 41742 B was discovered early on in the history of visual binaries, due to the brightness of the primary. The earliest measurement in the [[Wa ...ating that the star is a single-lined [[Binary star#Spectroscopic binaries|spectroscopic binary]] (SB1).<ref name="Lagrange2009"/> Though an orbital fit was not att ...

This is a single-lined [[spectroscopic binary]] system,<ref name=Abt2002/> which means that only the [[absorption | title=S_B⁹: The ninth catalogue of spectroscopic binary orbits ...

...on]] speed of stars. Speeds up to about 200 km/s are observed in eclipsing binaries. An exception is the fastest binary star, a rare type of two white dwarfs, ...particular brightness development, were actually binary stars (''eclipsing binaries'', like Algol).</ref> ...

| title=Automated spectroscopic abundances of A and F-type stars using echelle spectrographs. II. Abundance [[Category:Astrometric binaries]] ...

...s|disp=out}}.<ref name=tokovinin2008/> The primary component is itself a [[spectroscopic binary]] in a near circular orbit with a [[orbital period|period]] of aroun | title=Spectroscopic binary orbits from photoelectric radial velocities. Paper 104: 47 Cygni ...

Mu Ceti is a [[spectroscopic binary]]. These systems have binarity inferred from variations in their [[s ...the <var>μ</var> Cet Binary with Speckle Interferometric, Photometric, and Spectroscopic Techniques |journal=Astrophysical Bulletin |volume=79 |pages=445–463 |doi=1 ...

| title=Spectroscopic binaries among Hipparcos M giants. I. Data, orbits, and intrinsic variations ...

...|title=A study of the physical properties of SB2s with both the visual and spectroscopic orbits |bibcode=2020MNRAS.492.2709P |journal=Monthly Notices of the Royal A ...="Pourbaix2000">{{cite journal | title=Resolved double-lined spectroscopic binaries: A neglected source of hypothesis-free parallaxes and stellar masses | jour ...