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  • 1
    ISSN: 1432-0878
    Keywords: Key words Extraocular muscle ; Cation ; Muscular dystrophy ; Merosin ; dy Mouse
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Abstract Extraocular muscle is uniquely spared from damage in merosin-deficient congenital muscular dystrophy. Using a murine model, we have tested the hypothesis that the maintenance of calcium homeostasis is mechanistic in extraocular muscle protection. Atomic absorption spectroscopy has demonstrated a strong correlation between the perturbation of calcium homeostasis in hindlimb muscle that is severely damaged and the absence of changes in calcium in extraocular muscle. If, as in other skeletal muscles, extraocular muscle fibers are destabilized by merosin deficiency, we would expect an increase in total muscle calcium coupled with an adaptive response in the high capacity/speed of the sarcoplasmic reticulum of the eye muscle. However, we have not observed the expected increases in total muscle calcium content, Ca2+-ATPase activity, Na+/Ca2+ exchanger content, or smooth ER Ca2+-ATPase content that are predicted by this model. Instead, these results indicate that the increased membrane permeability that characterizes, and is potentially mechanistic in, myofiber degeneration in muscular dystrophy does not occur in merosin-deficient extraocular muscle. Thus, the high-capacity calcium-scavenging systems are not primarily responsible for extraocular muscle protection in muscular dystrophy.
    Type of Medium: Electronic Resource
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  • 2
    ISSN: 1432-0878
    Keywords: Key words Extraocular muscle ; Muscle development ; Myosin heavy chain ; Vestibular development ; Rat (Sprague Dawley)
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Abstract The genetic and epigenetic influences that establish and maintain the unique phenotype of the extraocular muscles (EOMs) are poorly understood. The vestibulo-ocular reflex (VOR) represents an important input into the EOMs, as it stabilizes eye position relative to the environment and provides a platform for function of all other eye movement systems. A role for vestibular cues in shaping EOM maturation was assessed in these studies using the ototoxic nitrile compound 3’,3’-iminodipropionitrile (IDPN) to eliminate the receptor hair cells that drive the vestibulo-ocular reflex. Intraperitoneal injections of IDPN were followed by a 2-week survival period, after which myosin heavy chain (MyHC) analysis of the EOMs was performed. When IDPN was administered to juvenile rats, the proportion of eye muscle fibers expressing developmental and fast myosins was increased, while EOM-specific MyHC mRNA levels were downregulated. By contrast, IDPN treatment in adult rats affected only the proportion of fibers expressing developmental MyHC isoforms, leaving the EOM-specific MyHC mRNA unaltered. These data provide evidence that the VOR modulates EOM-specific MyHC expression in development. The lack of significant changes in EOM-specific MyHC expression in adult EOM following IDPN administration suggests that there may be a critical period during development when alterations in vestibular activity have significant and permanent consequences for the eye muscles.
    Type of Medium: Electronic Resource
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  • 3
    Publication Date: 2019-07-18
    Description: Observations of cool DA and DB white dwarfs have not yet been successful in detecting coronal X-ray emission but observations of late-type dwarfs and giants show that coronae are common for these stars. To produce coronal X-rays, a star must have dynamo-generated surface magnetic fields and a well-developed convection zone. There is strong observational evidence that the DA star LHS 1038 and the DB star GD 358 have weak and variable surface magnetic fields. Since these fields are likely to be generated by dynamo action and since both stars have well-developed convection zones, theory predicts detectable levels of coronal X-rays from these white dwarfs. However, we present analysis of Chandra observations of both stars showing no detectable X-ray emission. The derived upper limits for the X-ray fluxes provide strong constraints on theories of formation of coronae around magnetic white dwarfs.
    Keywords: Astronomy
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  • 4
    Publication Date: 2019-07-13
    Description: Observational evidence for the existence of a chromosphere on the cool magnetic white dwarf GD 356 has been reported. In addition, there has been theoretical speculations that cool magnetic white dwarfs may be sources of coronal X-ray emission. This emission, if it exists, would be distinct from the two types of X-ray emission (deep photospheric and shocked wind) that have already been observed from hot white dwarfs. We have used the PSPC instrument on ROSAT to observe three of the most prominent DA white dwarf candidates for coronal X-ray emission: GD 356, KUV 2316+123, and GD 90. The data show no significant emission for these stars. The derived upper limits for the X-ray luminosities provide constraints for a revision of current theories of the generation of nonradiative energy in white dwarfs.
    Keywords: Astronomy
    Type: NASA-CR-203334 , NAS 1.26:203334 , The Astrophysical Journal; 453; L33-L35
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  • 5
    Publication Date: 2019-07-13
    Description: This paper will describe the scientific objectives of the Marshall Space Flight Center (MSFC) Solar Ultraviolet Magnetograph Investigation (SUMI) and the optical components that have been developed to meet those objectives. In order to test the scientific feasibility of measuring magnetic fields in the UV, a sounding rocket payload is being developed. This paper will discuss: (1) the scientific measurements that will be made by the SUMI sounding rocket program, (2) how the optics have been optimized for simultaneous measurements of two magnetic lines CIV (1550 Angstroms) and MgII (2800 Angstroms), and (3) the optical, reflectance, transmission and polarization measurements that have been made on the SUMI telescope mirror and polarimeter.
    Keywords: Astronomy
    Type: (ISSN 0277-786X)|Optical Characteristics of the Marshall Space Flight Center Solar Ultraviolet Magnetograph; Aug 01, 2001 - Aug 02, 2001; San Diego, CA; United States
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