"UY Scuti" pán-pún chi-kan bô-kāng--ê tē-hng
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Tē 1 chōa:
[[File:UY Scuti zoomed in, Rutherford Observatory, 07 September 2014.jpeg|thumb|[[Columbia Tāi-ha̍k]] ê [[Rutherfurd Thian-bûn-tâi]] hip--ê siòng-phìⁿ, tang-tiong siāng kng--ê tiō sī UY Scuti.]]
'''UY Scuti''' ('''BD-12 5055''') sī chi̍t lia̍p [[âng-sek chhiau-kī-chheⁿ]] (''red supergiant''), tiàm tī [[Scutum]] seng-chō. Pún chheⁿ sī só͘ chai-iáⁿ chiàu pòaⁿ-kèng sǹg siāng tōa ê [[hêng-chheⁿ]] chi it, chit-má ê [[chit-liōng]] sī {{solar mass|10}}.<ref name="Torres2013">{{Cite journal | last1 = Arroyo-Torres | first1 = B. | last2 = Wittkowski | first2 = M. | last3 = Marcaide | first3 = J. M. | last4 = Hauschildt | first4 = P. H. | title = The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii | doi = 10.1051/0004-6361/201220920 | journal = Astronomy & Astrophysics | volume = 554 | pages = A76 | year = 2013 | pmid = | pmc = | bibcode = 2013A&A...554A..76A |arxiv = 1305.6179 }}</ref>
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