Histopathology of Preclinical Toxicity Studies 2000
DOI: 10.1016/b978-044450514-9/50007-3
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Digestive System 1

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Cited by 4 publications
(4 citation statements)
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“…The lesions in the adrenal cortex (rats - hypertrophy and fatty degeneration in the cytoplasm of cells in the zona fasciculate) and in the non glandular and/or glandular stomach mucosa (rats and mice - erosions and/or ulceration and inflammation) were considered to be stress related (Greaves, 2000a; Greaves, 2000b). The presence of abnormal residual body formation in the high dose mouse testes was suggestive of a primary effect on the sustentacular Sertoli cells (Melnick et al, 2007).…”
Section: Discussionmentioning
confidence: 99%
“…The lesions in the adrenal cortex (rats - hypertrophy and fatty degeneration in the cytoplasm of cells in the zona fasciculate) and in the non glandular and/or glandular stomach mucosa (rats and mice - erosions and/or ulceration and inflammation) were considered to be stress related (Greaves, 2000a; Greaves, 2000b). The presence of abnormal residual body formation in the high dose mouse testes was suggestive of a primary effect on the sustentacular Sertoli cells (Melnick et al, 2007).…”
Section: Discussionmentioning
confidence: 99%
“…They are most commonly caused by antisecretory drugs (3,7,12,27,31,34) and are more common in rats than mice. This higher incidence in rats is probably because rats are more endowed with ECL cells, the cell type constituting the tumors (9). The mechanism of induction of carcinoids has been referred to as the "gastrin hypothesis" (3, 5, 7, 10-12, 17, 35).…”
Section: Discussionmentioning
confidence: 99%
“…In addition, neuroendocrine tumors rarely occur in control mice in standard 1.5-year CD-1 mouse oncogenicity studies. However, the chance of detecting this type of tumor is greater in extended 2-year studies (3,9). Background data on the spontaneous incidence of gastric neuroendocrine tumors in 2-year studies are scarce, and a single case, with metastasis to regional lymph nodes, was found in B6C3F1 mice (18,22).…”
Section: Discussionmentioning
confidence: 99%
“…Once (proto-)planets have been formed, they may significantly alter the surface density profile of the disk and thus cause signatures in the disk that are much easier to find than the planets themselves. The appearance and type of these signatures depend on the mass and orbit of the planet, but even more on the evolutionary stage of the circumstellar disk: While the spatial structure of optically thick, young circumstellar disks around Herbig AejBe and T Tauri stars is dominated by gas dynamics, the much lower optical depth and gas-to-dust mass ratios in debris disks (Zuckermann, Forveille, & Kastner 1995;Dent et al 1995;Artymowicz 1997;Liseau & Artymowicz 1998;Greaves, Coulson, & Holland 2000) let the stellar radiation via Poynting-Robertson effect and stellar wind drag, in addition to gravitation, be responsible for the resulting disk density distribution. Left: Azimuthally averaged disk surface density for planets with masses of 0.01 -1 MJupiter.…”
Section: Mapping Planet -Disk Interactionsmentioning
confidence: 99%