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  • ASTROPHYSICS  (1)
  • Arterial compliance  (1)
  • 2000-2004
  • 1985-1989  (2)
  • 1935-1939
  • 1985  (2)
  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Medical & biological engineering & computing 23 (1985), S. 197-202 
    ISSN: 1741-0444
    Keywords: Aortic dimensions ; Arterial compliance ; Arterial elasticity ; Ultrasonic aortography
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Chemistry and Pharmacology , Medicine
    Notes: Abstract The radii of the inner and outer walls of the aorta and the intravascular blood pressure were recorded simultaneously in the descending thoracic aorta of intact, living dogs using 7·5 MHz ultrasound. Blood pressure and the A-mode signals containing wall echoes were also recorded on videotape which was later replayed for processing. Thein vivo data were compared with data obtained on the same vessels post mortem. The change in radius due to a pressure change from 80 to 125 mmHg was calculated from thein vivo andin vitro data. After normalising the radius changes with respect to the radius at 80 mm Hg, the ratio of thein vivo andin vitro values ranged from 0·66 to 1·36 with a mean of 0·94. The changes in radius were comparable with previously reported values obtained using various techniques.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2019-06-28
    Description: A tool for exploring the evolution of X-ray emission from young SNRs is presented which employs a novel approach to the problem of time-dependent ionization in a shock-heated plasma. The solution of this problem is coupled to a spherically symmetric hydrodynamic calculation for the evolution of a point explosion in a uniform medium. The method is applied to Kepler's SNR, and two narrowly constrained classes of models which can simultaneously fit the spectral and morphological features of the object are found. One of these is a Sedov model in which the emission arises from shocked ambient gas, and the other is a reverse-shock model in which the SN ejecta is the dominant source of radiation. The emission from one specific model in each class is compared with the radial surface brightness profile, the 0.2-4.5 keV broadband spectrum, and the 1-3 keV moderate-resolution spectrum of the remnant. Reasonable fits are obtained in both cases.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 291; 544-560
    Format: text
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