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  • ASTRONOMY  (3)
  • Adenosine receptors  (1)
  • 2010-2014
  • 2000-2004
  • 1990-1994  (4)
  • 1965-1969
  • 1
    Digitale Medien
    Digitale Medien
    Springer
    Journal of comparative physiology 162 (1992), S. 179-183 
    ISSN: 1432-136X
    Schlagwort(e): Adenosine receptors ; Aortic smooth muscle ; dogfish shark, Squalus acanthias
    Quelle: Springer Online Journal Archives 1860-2000
    Thema: Biologie , Medizin
    Notizen: Summary Isolated, endothelium-free rings of vascular smooth muscle (VSM) from the ventral aorta of the dogfish shark, Squalus acanthias, were used to examine the vasoactive effects of various adenosine agonists. Cumulative addition of 2-chloroadenosine (2 Cl-ADO) over the concentration range 10 nM–1 mM resulted in a biphasic response, with a significant increase in tension at 1 μM and a more significant decline in tension at 100 μM and 1 mM, suggesting that this tissue may possess both A1 and A2 adenosine receptors. N6-Cyclopentyladenosine (N-6 CPA) and N6-(2-phenylisopropyl)adenosine, R(-)isomer (R-PIA), generally considered to be more A1 specific, also produced slight, but significant increases in tension, but only at relatively high concentrations. The more specific A1 agonist, N6-(25)-[2-endo-norbonyl] adenosine [(S)-ENBA] produced a significant increase in tension at 1 pM, reaching 28% above control at 10 nM. The response to (S)-ENBA was also biphasic, with a fall in tension at 10 μM. The relatively non-specific agonist 5′-N-ethylcarboxamidoadenosine (NECA) produced a small, but significant, increase in tension at 1 μM, with no subsequent decline in tension at higher concentrations. These results allow us to assign a tentative structure-activity relationship (SAR) for an increase in tension of (S)-ENBA≫R-PIA≥2-Cl ADO=N-6 CPA=NECA; for the decrease, the SAR is (S)-ENBA〉2-Cl ADO〉R-PIA〉N-6 CPA=NECA. These SARs are consistent with the hypothesis that the VSM from the ventral aorta of this elasmobranch fish contains both A1 and A2 adenosine receptors. This is the first such description of both adenosine receptors in fish VSM. The role of a putative release of adenosine from the fish heart on branchial hemodynamics remains to be determined.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 2
    Publikationsdatum: 2019-06-28
    Beschreibung: Planetary Radio Astronomy (PRA) data from the Voyager Neptune encounter were cleaned and reformatted in a variety of formats. Most of these formats are new and have been specifically designed to provide easy access and use of the data without the need to understand esoteric characteristics of the PRA instrument or the Voyager spacecraft. Several data sets were submitted to the Planetary Data System (PDS) and have either appeared already on peer reviewed CDROM's or are in the process of being reviewed for inclusion in forthcoming CD-ROM's. Many of the data sets are also available online electronically through computer networks; it is anticipated that as time permits, the PDS will make all the data sets that were a part of this contract available both online and on CD-ROM's.
    Schlagwort(e): ASTRONOMY
    Materialart: NASA-CR-193261 , NAS 1.26:193261
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 3
    Publikationsdatum: 2019-07-13
    Beschreibung: The Planetary Radio Astronomy (PRA) instrument detected large numbers of dust particles during the Voyager 2 encounter with Neptune. The signatures of these impacts are analyzed in some detail. The major conclusions are described. PRA detects impacts from all over the spacecraft body, not just the PRA antennas. The signatures of individual impacts last substantially longer than was expected from complementary Plasma Wave Subsystem (PWS) data acquired by another Voyager experiment. The signatures of individual impacts demonstrate very rapid fluctuations in signal strength, so fast that the data are limited by the speed of response of the instrument. The PRA detects events at a rate consistently lower than does the Plasma Wave subsystem. Even so, the impact rate is so great near the inbound crossing of the ring plane that no reliable estimate of impact rate can be made for this period. The data are consistent with the presence of electrons accelerated by ions within an expanding plasma cloud from the point of impact. An ancillary conclusion is that the anomalous appearance of data acquired at 900 kHz appears to be due to an error in processing the PRA data prior to their delivery rather than due to overload of the PRA instrument.
    Schlagwort(e): ASTRONOMY
    Materialart: NASA-CR-193281 , NAS 1.26:193281
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 4
    Publikationsdatum: 2019-07-12
    Beschreibung: The analysis and results of an occultation of the spectroscopic binary star 1 Vulpeculae by the asteroid (2) Pallas, observed from 130 locations, are presented. Combination of solutions from this and previous occultations shows the triaxial shape of Pallas to be elongated, but not severely, with the ratio of the largest to the smallest axes being less than 1.15. The data provide a separation and a position angle of the secondary component of 1 Vulpeculae and indicate that the star's actual parallax is probably near 0.008 arcsec, half of the published value. The analysis gives a calibration of the accuracy and the reaction time corrections for visual observations of asteroidal occultations. The absence of any confirmed secondary extinctions shows that any satellites of Pallas must be rare or small. The photometric observations seem to rule out a substantial cloud of dust surrounding Pallas postulated previously.
    Schlagwort(e): ASTRONOMY
    Materialart: Astronomical Journal (ISSN 0004-6256); 99; 1636-166
    Format: text
    Standort Signatur Erwartet Verfügbarkeit
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