Primary irsi stromal cyst:A report of 17 cases

Objective: To describe clinical characteristics, management, and complications of primary iris stromal cysts. Design: A retrospective review. Results: Seventeen consecutive patients with primary iris stromal cysts were found. Nine (52%) patients were diagnosed under age 10 years (range, 1 day-7 years), and eight (47%) patients were diagnosed after age 10 years (range, 14-71 years). Overall, the cyst appeared unilaterally as a solitary clear translucent mass dissecting the iris stroma in all cases. The children with a primary iris stromal cyst demonstrated a more aggressive course than teenagers or adults. In children, the cyst obstructed the visual axis in eight cases (88%), requiring treatment such as aspiration, cryotherapy, and resection. In seven children, multiple treatments were necessary. Ultimate control of the cyst was achieved in all cases using techniques of needle aspiration (with or without cryotherapy) in three cases and using resection in five cases. Primary iris stromal cysts in teenagers and adults necessitated intervention in only two cases (25%). Conclusion: Primary iris stromal cysts can occur in children, teenagers, and adults. In children, primary stromal iris cysts appear to have a more aggressive clinical course, often requiring several treatments for globe and vision preservation.

Dual-colour HER2/chromosome 17 chromogenic in situ hybridisation enables accurate assessment of HER2 genomic status in ovarian tumours

Ovarian cancer is a leading cause of gynaecological cancer-related morbidity and mortality. There has been increasing interest in the potential utility of anti-human epidermal growth factor receptor 2 (anti-HER2) agents in the treatment of this disease, with the attendant need to identify suitable predictive biomarkers of response to treatment.

Dual-colour HER2/chromosome 17 chromogenic in situ hybridisation assay enables accurate assessment of HER2 genomic status in gastric cancer and has potential utility in HER2 testing of biopsy samples

Determination of HER2 protein expression by immunohistochemistry (IHC) and genomic status by fluorescent in situ hybridisation (FISH) are important in identifying a subset of high HER2-expressing gastric cancers that might respond to trastuzumab. Although FISH is considered the standard for determination of HER2 genomic status, brightfield ISH is being increasingly recognised as a viable alternative. Also, the impact of HER2 protein expression/genomic heterogeneity on the accuracy of HER2 testing has not been well studied in the context of gastric biopsy samples.

EL CVn-type binaries - Discovery of 17 helium white dwarf precursors in bright eclipsing binary star systems

The star 1SWASP J024743.37-251549.2 was recently discovered to be a binary star in which an A-type dwarf star eclipses the remnant of a disrupted red giant star (WASP 0247-25 B). The remnant is in a rarely observed state evolving to higher effective temperatures at nearly constant luminosity prior to becoming a very low mass white dwarf composed almost entirely of helium, i.e. it is a pre-helium white dwarf (pre-He-WD). We have used the photometric database from theWide Angle Search for Planets (WASP) to find 17 eclipsing binary stars with orbital periods P = 0.7-2.2 d with similar light curves to 1SWASP J024743.37-251549.2. The only star in this group previously identified as a variable star is the brightest one, EL CVn, which we adopt as the prototype for this class of eclipsing binary star. The characteristic light curves of EL CVn-type stars show a total eclipse by an A-type dwarf star of a smaller, hotter star and a secondary eclipse of comparable depth to the primary eclipse. We have used new spectroscopic observations for six of these systems to confirm that the companions to the A-type stars in these binaries have very low masses (≈0.2M⊙). This includes the companion to EL CVn which was not previously known to be a pre-He-WD. EL CVn-type binary star systems will enable us to study the formation of very low mass white dwarfs in great detail, particularly in those cases where the pre-He-WD star shows non-radial pulsations similar to those recently discovered in WASP0247-25 B. © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.