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  • 1
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Berichte der deutschen chemischen Gesellschaft 92 (1959), S. 1765-1771 
    ISSN: 0009-2940
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Reaktionen des Mangancarbonyls mit Phosphinen führen zu Monosubstitutionsprodukten, entspr. Mn(CO)4PR3, die je nach der Natur des Restes R ein- oder zweikernig gebaut sind. Einkernige, paramagnetische Verbindungen leiten sich von Triphenyl- oder Triäthylphosphin und den homologen Arsinen und Stibinen ab, während mit Tricyclohexylphosphin und Triphenylphosphit diamagnetische, zweikernige Derivate entstehen; in Lösung ist häufig ein temperaturabhängiges Gleichgewicht zwischen der monomeren und der dimeren Form anzunehmen. Auf Grund von IR-Spektren und Dipolmessungen wird der räumliche Bau der Verbindungen erörtert.
    Additional Material: 8 Ill.
    Type of Medium: Electronic Resource
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  • 2
    ISSN: 0009-2940
    Keywords: AM1 calculations ; Chloralide ; Dioxolane ; Force-field calculations ; Tartaric acid ; Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Isolation of a third diastereoisomer (1c) of (R,R)-tartaric acid chloralide is described. A comparison of structural data derived by X-ray analysis with calculated parameters is given. Structures are generated by the ALCHEMY force-field program as well as by AM1 calculations.
    Additional Material: 3 Ill.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Berichte der deutschen chemischen Gesellschaft 91 (1958), S. 2824-2829 
    ISSN: 0009-2940
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Durch Tritylierung und Acetylierung der Saccharose wird eine Tritrityl-penta-acetyl-saccharose und daraus durch Tritylabspaltung eine Pentaacetyl-saccharose erhalten, die durch Acetylwanderung eine Iso-pentaacetyl-saccharose liefert. Die Konstitution beider Pentaacetate wird bewiesen.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Berichte der deutschen chemischen Gesellschaft 91 (1958), S. 1230-1234 
    ISSN: 0009-2940
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Die Reaktion des Kobaltcarbonyls mit Triphenylphosphin in polaren Mitteln wie Dioxan (bei 30°) führt im Sinne der Disproportionierung 2 Co° → Co⊕ + Co⊖ zu einer 2-ionigen Verbindung [CoI(CO)3(P(C6H5)3)2]⊕[Co-I(CO)4]⊖, die sich mit Komplexen wie [B(C6H5)4]⊖, [HgJ4]2⊖, [Cr(NH3)2(SCN)4]⊖ unter Bildung entspr. Salze des Tricarbonyl-bis-[triphenylphosphin]-Kations umsetzen läßt. Außerdem entsteht, besonders in indifferenten Mitteln (bei 0°), als echtes Derivat des Kobalttetracarbonyls das bisher allein bekannte Bis-[tric-carbonyl-triphenylphosphin-kobalt(0)], [Co(CO)3P(C6H5)3]2; häufig liegen Gemenge beider Verbindungen vor. - Die magnetochemische Untersuchung ergibt für die ionogene Verbindung Diamagnetismus, das Kation ist somit ein Durchdringungskomplex edelgasähnlicher Konfiguration; das Reinecke-Salz zeigt dementsprechend den Paramagnetismus den komplexen Chromat(III)-Anions. Der Diamagnetismus des Substitutionsproduktes beweist dessen zweikernige Struktur, wie sie schon bisher postuliert wurde.
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  • 5
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Berichte der deutschen chemischen Gesellschaft 90 (1957), S. 2023-2024 
    ISSN: 0009-2940
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 6
    ISSN: 0009-2940
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Unter Anwendung einer kürzlich neu aufgefundenen, ohne Katalysator gemäß \documentclass{article}\pagestyle{empty}\begin{document}$$ {\rm Me}\left({{\rm CO}} \right)_6 + {\rm Ar} \to {\rm ArMe}\left({{\rm CO}} \right)_3 + 3\,{\rm CO} $$\end{document} \documentclass{article}\pagestyle{empty}\begin{document}$$\left({{\rm Me} = {\rm Cr},\,{\rm Mo},\,{\rm W};{\rm Ar} = {\rm C}_6 {\rm H}_6 {\rm und}\,{\rm Derivate}} \right) $$\end{document} bei erhöhter Temperatur verlaufenden Synthese wurden zahlreiche gemischte Sechsringaromaten-Metallcarbonyle von Cr, Mo und W dargestellt. Neben Benzol, seinen Alkylverbindungen und Naphthalin als kondensiertem Aromaten erwiesen sich auch Derivate mit einsamen Elektronenpaaren in der funktionellen Gruppe, wie z. B. C6H5Cl, C6H5OH, C6H5NH2, C6H5CO2CH3, als der π-Komplexbildung fähig. Aus CH3O2CC6H5Cr(CO)3 wurde durch alkalische Verseifung weiterhin HO2CC6H5Cr(CO)3 erhalten. Die meist gelben, sublimierbaren, diamagnetischen Verbindungen sind ebenso wie C6H6Cr(CO)3 und C4H4SCr(CO)3 als edelgaskonfigurierte Durchdringungs-komplexe mit zentralem, sechsbindigem Me0 aufzufassen.  -  Die an \documentclass{article}\pagestyle{empty}\begin{document}$$ {\rm C}_6 {\rm H}_5 {\rm OHCr}\left({{\rm CO}} \right)_3,{\rm C}_6 {\rm H}_5 {\rm CO}_2 {\rm HCr}\left({{\rm CO}} \right)_3 \,{\rm und}\,{\rm C}_6 {\rm H}_5 {\rm NH}_2 {\rm Cr}\left({{\rm CO}} \right)_3 $$\end{document} gegenüber den jeweiligen freien Aromaten auftretende Aciditätssteigerung bzw. Basizitätsverminderung entspricht einem induktiven Effekt, der durch die Einbeziehung des π-Elektronensextetts in die Metallschale zustandekommt.
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  • 7
    facet.materialart.
    Unknown
    In:  Other Sources
    Publication Date: 2011-08-19
    Description: Observations covering a period of 20 years show that the large proper motion (4.08 arcsec/yr) of the nearly triple system 40 Eridani-ABC will cause its brightest member, A, to pass within 3 arcsec of a faint background star. The originally hoped-for primary gravitational lens effect will therefore not take place although a minor secondary effect may occur near the time of closest approach on June 1, 1987.
    Keywords: ASTRONOMY
    Type: Astronomical Society of the Pacific, Publications (ISSN 0004-6280); 98; 1199
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  • 8
    facet.materialart.
    Unknown
    In:  CASI
    Publication Date: 2013-08-31
    Description: High-resolution IUE spectra of the Mg II k line of HD 199178 were analyzed, applying spectral imaging techniques to derive an image of the chromospheric structure and to study the transient behavior of the chromosphere. All spectra in the IUE archives were uniformly reduced and analyzed. Results are compared with ground-based observations of the photosphere. Four ultraviolet flares on HD 199178 are observed; 3 of these occurred at roughly the same rotational phase. There is no clear phase-dependence of the SWP line fluxes, but there is for the Mg II k flux. The emission centroid of the Mg II k line varies in a quasi-sinusoidal fashion, presumably due to the rotation of a nonuniform chromosphere.
    Keywords: ASTRONOMY
    Type: ESA, A Decade of UV Astronomy with the IUE Satellite, Volume 1; p 291-293
    Format: application/pdf
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  • 9
    Publication Date: 2013-08-29
    Description: The spatially unresolved emission line object AS 201 was observed by IUE in the low dispersion mode. It shows a UV spectrum similar to that of planetary nebulae or symbiotic stars. The optical spectrum shows characteristics of a G2 III star, but the UV indicates that a hot companion is present, as evidenced by strong C III, C IV, and moderately strong He II emissions. A fairly strong continuum is also seen throughout the IUE range. The log R (I(C III)/I(Si III)) value of 1.44 strongly argues for AS 201 being a planetary nebula and not a symbiotic star.
    Keywords: ASTRONOMY
    Type: ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2; p 179-181
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  • 10
    Publication Date: 2011-08-19
    Description: Low-dispersion IUE spectra confirm that the emission-line object Cn 1-2 is a symbiotic star and not a planetary nebula. The UV spectrum of Cn 1-2 strongly resembles those of V1016 Cyg and HM Sge. The object is correctly identified in the finder field of Allen's Catalogue of Symbiotic Stars (1984) but misidentified in the Catalogue of Galactic Planetary Nebulae by Perek and Kohoutek (1967).
    Keywords: ASTRONOMY
    Type: Astronomical Society of the Pacific, Publications (ISSN 0004-6280); 100; 1101-110
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