Publications by authors named "Bosh A"

Recent spacecraft and radar observations have found that ~70 percent of short-period comet nuclei, mostly Jupiter-family comets (JFCs), have bilobate shapes (two masses connected by a narrow neck). This is in stark contrast to the shapes of asteroids of similar sizes, of which ~14% are bilobate. This suggests that a process or mechanism unique to comets is producing these shapes.

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The Kuiper belt is a collection of small bodies (Kuiper belt objects, KBOs) that lie beyond the orbit of Neptune and which are believed to have formed contemporaneously with the planets. Their small size and great distance make them difficult to study. KBO 55636 (2002 TX(300)) is a member of the water-ice-rich Haumea KBO collisional family.

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Three new triterpene glycosides, achlioniceosides A(1) (1), A(2) (2), and A(3) (3), have been isolated from the Antarctic sea cucumber Achlionice violaecuspidata. The glycoside structures were elucidated using extensive NMR spectroscopic analysis including one-dimensional (1)H and (13)C spectra, (1)H-(1)H-COSY, HMBC, HMQC, and NOESY and mass spectrometry. Gycosides 1-3 are disulfated pentaosides that are branched at the first xylose residue.

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Hypertrophic cardiomyopathies (HCM) are a frequent cause of sudden death in both young people and adults. Different cardiomyopathies can be distinguished according to the etiological agent and, although there are morphological differences too, alterations in the quantity of DNA in the cardiomyocytes may play an important role in their pathogenesis and evolution. To understand the characteristics and the behaviour of the DNA index in hypertrophic cardiomyopathies, we have studied thirty cases (10 primaries or essential, 10 hypertensives and 10 toxic) and compared the results with those obtained for 10 macroscopically normal hearts.

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Stellar occultations--the passing of a relatively nearby body in front of a background star--can be used to probe the atmosphere of the closer body with a spatial resolution of a few kilometres (ref. 1). Such observations can yield the scale height, temperature profile, and other information about the structure of the occulting atmosphere.

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