2012
DOI: 10.4235/jkgs.2012.16.4.221
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Purple Urine Bag Syndrome

Abstract: Purple urine bag syndrome (PUBS) is a rare condition, in which the patient has a purple-colored urine tubes or bags following urinary catheterization for hours to months. It is usually associated with elderly females, prolonged urinary catheterization, some bacterial infections that produce sulphatase/phosphatase, chronic debilitated state, and chronic constipation. We present a case report of this rare phenomenon occurring in a 73-year-old woman.

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Cited by 5 publications
(10 citation statements)
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“…[6][7][8][9] Proposed risk factors are a long-term indwelling urinary catheter, female sex, older age, and the presence of chronic constipation, chronic renal disease, bedridden state, alkaline urine, and urinary tract infection. 1,5,10,11) The pathogenesis of PUBS is summarized in Fig. 2.…”
Section: Discussionmentioning
confidence: 99%
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“…[6][7][8][9] Proposed risk factors are a long-term indwelling urinary catheter, female sex, older age, and the presence of chronic constipation, chronic renal disease, bedridden state, alkaline urine, and urinary tract infection. 1,5,10,11) The pathogenesis of PUBS is summarized in Fig. 2.…”
Section: Discussionmentioning
confidence: 99%
“…These pigments mix and react with the urine bag and tubing and produce a purple-colored urine. 1,5,[11][12][13] Several bacteria are often associated with PUBS. These bacteria are mainly gram negative and include Providencia rettgeri, Providencia stuartii, Proteus mirabilis, Klebsiella pneumonia, Enterococcus species, Escherichia coli, Morganella morganii, Pseudomonas aeruginosa, Citrobacter species, and group B streptococci.…”
Section: Discussionmentioning
confidence: 99%
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“…We examined the process of EW measurement performed by TAME with the actual spectra of HD 75732 ([Fe/H] = +0.35) as a metalrich star and HD 155358 ([Fe/H] = −0.63) as a relatively metal-poor star. These spectra were obtained at Bohyunsan Optical Astronomy Observatory (BOAO) with the BOAO Echelle Spectrograph (BOES) (Kim et al 2002(Kim et al , 2007 in 2008 and have the spectral resolution R = 30 000 and an S/N ratio of ∼200 (Kang et al 2011). Fig.…”
Section: Examples Using the Spectra Of Metal-rich And Metal-poor Starsmentioning
confidence: 99%