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1.
Ir Vet J ; 61(3): 163-8, 2008 Mar 01.
Article in English | MEDLINE | ID: mdl-21851709

ABSTRACT

The deposition of semen, bacteria and debris in the uterus of the mare after breeding normally induces a self-limiting endometritis. The resultant fluid and inflammatory products are cleared by 48 hours post cover. Mares that are susceptible to persistent post-breeding endometritis (PPBEM) have impaired uterine defence and clearance mechanisms, making them unable to resolve this inflammation within the normal time. This persists beyond 48 hours post-breeding and causes persistent fluid accumulation within the uterus. Mares with PPBEM have an increased rate of embryonic loss and a lower overall pregnancy rate than those without the condition. To enhance conception rates, mares at high risk need optimal breeding management as well as early diagnosis, followed by the most appropriate treatment. This article reviews the pathogenesis, diagnosis and treatment of PPBEM and the management of affected mares.

2.
Astrophys J ; 533(1): L25-L28, 2000 Apr 10.
Article in English | MEDLINE | ID: mdl-10727383

ABSTRACT

The Dominion Radio Astrophysical Observatory's Synthesis Telescope provides the highest resolution data (1&arcmin; and 0.82 km s-1) to date of an H i worm candidate. Observed as part of the Canadian Galactic Plane Survey, mushroom-shaped GW 123.4-1.5 extends only a few hundred parsecs, contains approximately 105 M middle dot in circle of neutral hydrogen, and appears unrelated to a conventional shell or chimney structure. Our preliminary Zeus two-dimensional models use a single off-plane explosion with a modest ( approximately 1051 ergs) energy input. These generic simulations generate, interior to an expanding outer blast wave, a buoyant cloud whose structure resembles the morphology of the observed feature. Unlike typical model superbubbles, the stem can be narrow because its width is not governed by the pressure behind the blast wave or the disk scale height. Using this type of approach, it should be possible to more accurately model the thin stem and other details of GW 123.4-1.5 in the future.

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