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  • 1
    ISSN: 1432-1041
    Keywords: beta-blocking drugs ; coronary artery disease ; myocardial infarction ; haemodynamic response
    Source: Springer Online Journal Archives 1860-2000
    Topics: Chemistry and Pharmacology , Medicine
    Notes: Summary Theoretically the increased sympathoadrenal activity following acute myocardial infarction might augment the haemodynamic impact of beta-adrenoceptor blockade. To evaluate this question 32 haemodynamic studies were performed to compare the effects of equivalent beta-blocking doses of propranolol (8 mg i.v.) and pindolol (0.8 mg i.v.) in patients with a recent acute myocardial infarction (A.M.I.) or stable coronary artery disease (and a presumptive low sympathetic state). In stable coronary artery disease there were clear differences between the haemodynamic impact of propranolol and pindolol. Propranolol decreased both heart rate (ΔHR −7 beat/min) and cardiac index (ΔCI −0.4l/min/m2), with an increased pulmonary artery occluded pressure (ΔPAOP +4 mmHg) and systemic vascular resistance index (ΔSVRI +358 dyn · s · cm−5 m2). However an equivalent beta-blocking dose of pindolol increased PAOP (ΔPAOP +3 mmHg) leaving other variables unchanged. These differential actions of propranolol and pindolol have previously been ascribed to the intrinsic synpathomimetic activity (I.S.A.) of pindolol maintaining cardiac pumping function in a low sympathetic state. In contrast following myocardial infarction, both drugs reduced cardiac index to a significantly greater extent compared with stable coronary artery disease (ΔCI propranolol −0.8l/min/m2; pindolol −0.4l/min/m2;p〈0.05); propranolol also reduced the systemic arterial blood pressure (Δsystolic −10 mmHg; Δmean −5 mmHg;p〈0.05). The haemodynamic relevance of the I.S.A. of pindolol appeared attenuated following A.M.I. These data are compatible with experimental evidence of sympathetic nervous activation following coronary occlusion; the resulting hyperadrenergic state appears to condition an augmented haemodynamic response to beta-blocking drugs irrespective of their ancillary pharmacological properties. The implications of these findings for clinical therapy warrant further examination.
    Type of Medium: Electronic Resource
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  • 2
    ISSN: 1432-1041
    Keywords: beta-receptor blocking drugs ; myocardial infarction ; haemodynamic effects ; propranolol ; pindolol ; intrinsic sympathomimetic activity
    Source: Springer Online Journal Archives 1860-2000
    Topics: Chemistry and Pharmacology , Medicine
    Notes: Summary The relevance of the intrinsic sympathomimetic activity (ISA) of beta-blocking compounds to the clinical therapeutics of acute myocardial infarction was evaluated in 20 patients with an uncomplicated acute myocardial infarction by comparing the haemodynamic effects of equivalent beta-blocking doses of propranolol (non-cardioselective; no ISA) and pindolol (non-cardioselective; 50% ISA). Consecutive eligible male patients admitted to a Coronary Care Unit were randomised following a 1 h control period to two separate studies. In Study 1 the short-term dose-response effects of propranolol (1–8 mg) or pindolol (0.1–0.8 mg) were assessed. In Study 2 comparison of the effects of single i.v. propranolol (8 mg) and pindolol (0.8 mg) doses was undertaken over 6 h. Haemodynamic variables and thermodilution cardiac output were subsequently recorded to compare the effects of each drug on the circulation. The plasma concentrations of propranolol and pindolol were in the recognised therapeutic range. Both drugs were clinically well-tolerated, the changes induced in haemodynamic variables following each drug demonstrated effective beta-blockade. Within the limits of the experimental protocol, these data did not suggest definite haemodynamic advantage for ISA of pindolol in acute myocardial infarction. These findings are perhaps due to sympathetic activation in acute myocardial infarction attenuating the haemodynamic impact of ISA.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    European journal of clinical pharmacology 24 (1983), S. 747-750 
    ISSN: 1432-1041
    Keywords: sulphinpyrazone ; myocardial infarction ; renal function ; uric acid excretion ; prognostic implications
    Source: Springer Online Journal Archives 1860-2000
    Topics: Chemistry and Pharmacology , Medicine
    Notes: Summary The effects of sulphinpyrazone 800 mg daily on renal excretory function were studied in a double-blind placebo-controlled randomised trial of incremental and full doses of the drug in 28 patients with plasma urea concentration 〈10 mmol/l in the period 2–28 days following uncomplicated acute myocardial infarction. Sulphinpyrazone in both dosage regimens increased uric acid excretion and lowered plasma urate concentration. There was no evidence that the drug reduced glomerular filtration rate or damaged the renal tubules. These results suggest that sulphinpyrazone in the doses used in this study is not contraindicated in patients early after acute myocardial infarction even though they may have a moderate rise in the blood urea.
    Type of Medium: Electronic Resource
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  • 4
    Publication Date: 2013-08-31
    Description: The abundance pattern of siderophile elements in terrestrial and lunar impact melt rocks was used extensively to infer the nature of the impacting projectiles. An implicit assumption made is that the siderophile abundance ratios of the projectiles are approximately preserved during mixing of the projectile constituents with the impact melts. As this mixture occurs during flow of strongly shocked materials at high temperatures, however there are grounds for suspecting that the underlying assumption is not always valid. In particular, fractionation of the melted and partly vaporized material of the projectile might be expected because of differences in volatility, solubility in silicate melts, and other characteristics of the constituent elements. Impactites from craters with associated meteorites offer special opportunities to test the assumptions on which projectile identifications are based and to study chemical fractionation that occurred during the impact process.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1990; p 375-376
    Format: application/pdf
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  • 5
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    In:  Other Sources
    Publication Date: 2019-01-25
    Description: The concept that the Moon was fissioned from the Earth after core separation is the most readily testable hypothesis of lunar origin, since direct comparisons of lunar and terrestrial compositions can be made. Differences found in such comparisons introduce so many ad hoc adjustments to the fission hypothesis that it becomes untestable. Further constraints may be obtained from attempting to date the volatile-refractory element fractionation. The combination of chemical and isotopic problems suggests that the fission hypothesis is no longer viable, and separate terrestrial and lunar accretion from a population of fractionated precursor planetesimals provides a more reasonable explanation.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Planetary Inst. Conf. on the Origin of the Moon; p 25
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  • 6
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    In:  Other Sources
    Publication Date: 2019-01-25
    Description: The development of planetary crusts may be divided into primary, resulting from melting during accretion, and secondary crusts developed by partial melting from planetary mantles. The Mercurian crust is probably primary with no compelling evidence of later basaltic extrusions. Reflectance spectral evidence for the existence Fe2(+) is equivocal. The Viking Lander XRF data on Mars indicate basaltic material at both sites 4,000 km apart. Surface aeolian processes would be expected to provide a homogeneous average of the crust, but no evidence of more siliceous material is present. This conclusion is weakly supported by the Russian gamma ray data. No evidence for granite appears from the Russian Venera XRF data which indicates MORB-type and alkali basalt (4% K2O) surface compositions. The highlands of Ishtar Terra and Aphrodite probably owe their elevation to tectonic processes rather than compositional effects. Venus may thus resemble the early Archean Earth. The terrestrial granitic continental crust is a product of episodic multiple partial melting events, probably a consequence of the presence of surface water.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Inst. Terrest. Planets: Comp. Planetology; p 15
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  • 7
    Publication Date: 2019-06-28
    Description: The ages of the earth and moon as determined by various chronometric systems are discussed with primary emphasis placed on the development of an I-Pu-Xe chronometer. Data on excess fission xenon are reviewed with attention given to the strengths and weaknesses of the assumptions required for lunar I-Pu-Xe chronometry. Using I-Pu-Xe dating, it is estimated that the retention of excess fission xenon in lunar samples began no more than 63 + or - 42 m.y. after the time of primitive meteorite formation.
    Keywords: LUNAR AND PLANETARY EXPLORATION
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  • 8
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    Publication Date: 2019-06-28
    Description: An interpretative synthesis of current knowledge on the moon and the terrestrial planets is presented, emphasizing the impact of recent lunar research (using Apollo data and samples) on theories of planetary morphology and evolution. Chapters are included on the exploration of the solar system; geology and stratigraphy; meteorite impacts, craters, and multiring basins; planetary surfaces; planetary crusts; basaltic volcanism; planetary interiors; the chemical composition of the planets; the origin and evolution of the moon and planets; and the significance of lunar and planetary exploration. Photographs, drawings, graphs, tables of quantitative data, and a glossary are provided.
    Keywords: LUNAR AND PLANETARY EXPLORATION
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  • 9
    Publication Date: 2019-07-13
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Science Conference; Mar 14, 1977 - Mar 18, 1977; Houston, TX
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  • 10
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    In:  Other Sources
    Publication Date: 2019-07-13
    Description: Evidence for and implications of homogeneous accretion of the moon are considered. Interelement ratios are used to calculate the composition of the highland crust. The rare-earth data for the highlands show a positive Eu anomaly, allowing the deduction that the interior has a negative anomaly. The Cr/Ni ratios in the highlands are considered in regard to the overall lunar abundance of the siderophile elements. These abundance data and the constraints from the heat flow measurements are next used to set limits on the bulk composition for the moon. The geochemical constraints are integrated with the petrological and geophysical data in an attempt to provide a consistent model for the geochemical evolution of the moon.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Science Conference; Mar 18, 1974 - Mar 22, 1974; Houston, TX
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