T Centauri
{{Short description|Variable star in the constellation Centaurus}}
{{distinguish|Tau Centauri|Theta Centauri}}
{{Starbox begin}}
{{Starbox observe
| epoch = J2000.0
| constell = Centaurus
| dec = {{DEC|-33|35|50.5600}}
}}
{{Starbox character
| variable = semiregular
}}
{{Starbox astrometry
| radial_v = {{val|+32.6|2.5}}
| prop_mo_ra = −27.747
| prop_mo_dec = +3.365
| parallax = 2.4007
| p_error = 0.0687
}}
{{Starbox catalog
| names={{odlist|V=T Cen|CD=-32°9549|HD=119090|HIP=66825|HR=5147|SAO=204739}}
}}
{{Starbox reference|Simbad=T+Cen}}
{{Starbox end}}
File:TCenLightCurve.png light curve for T Centauri, plotted from ASAS data]]
T Centauri is a variable star located in the far southern constellation Centaurus. It varies between magnitudes 5.56 and 8.44 over 181.4 days, making it intermittently visible to the naked eye. Pulsating between spectral classes K0:e and M4II:e, it has been classed as a semiregular variable, though Sebastian Otero of the American Association of Variable Star Observers has noted its curve more aligned with RV Tauri variable stars and has classified it as one.
The variability of the star was discovered in 1894 by Ernest Elliott Markwick, and independently by Williamina Fleming in 1895.
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References
{{reflist|refs=
{{cite simbad |title=T Centauri |access-date=2025-05-25 }}
{{cite Gaia DR3|6165341341986059520}}
{{cite web|url=http://www.aavso.org/vsx/index.php?view=detail.top&oid=7300 |title=T Centauri |author =Watson, Christopher |date=27 December 2012 |work=AAVSO Website|publisher=American Association of Variable Star Observers|access-date=22 July 2014}}
}}
{{Stars of Centaurus}}
{{DEFAULTSORT:T Centauri}}
Category:Semiregular variable stars
Category:Durchmusterung objects
Category:Asymptotic-giant-branch stars
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