1980
DOI: 10.1107/s0567740880006309
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Structure of calcium nitroprusside tetrahydrate

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1980
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Cited by 15 publications
(3 citation statements)
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“…Absorption spectra of CC2DNB and CC3 DNB were recorded in 100 m M HEPES buffer (pH 7.4, Figure 2 a) and methanol (Figure 2 b), and compared with those of CCDNB under similar conditions. The reported absorption maxima of 348 nm for free N ‐ethyl‐substituted 2,4‐dinitroaniline8 and of 362 nm for 1‐(methylthio)‐2,4‐dinitrobenzene9 in methanol are quite similar to the observed absorption peaks at 350 nm in methanol for the synthesized probes containing the DNB part. In aqueous buffer, the absorption maxima for the coumarin and DNB parts of both CCDNB and CC2DNB were observed at 407 nm and 375 nm, respectively.…”
Section: Fluorescence Quantum Yields Of the Synthesized Probes In Bufsupporting
confidence: 68%
“…Absorption spectra of CC2DNB and CC3 DNB were recorded in 100 m M HEPES buffer (pH 7.4, Figure 2 a) and methanol (Figure 2 b), and compared with those of CCDNB under similar conditions. The reported absorption maxima of 348 nm for free N ‐ethyl‐substituted 2,4‐dinitroaniline8 and of 362 nm for 1‐(methylthio)‐2,4‐dinitrobenzene9 in methanol are quite similar to the observed absorption peaks at 350 nm in methanol for the synthesized probes containing the DNB part. In aqueous buffer, the absorption maxima for the coumarin and DNB parts of both CCDNB and CC2DNB were observed at 407 nm and 375 nm, respectively.…”
Section: Fluorescence Quantum Yields Of the Synthesized Probes In Bufsupporting
confidence: 68%
“…Aymonino, Baran, Gentil, Lanfranconi & Varetti, 1976;Castellano, Piro & Rivero, 1977a,b;Castellano, Piro, Podjarny, Rivero, Aymonino, Lesk & Varetti, 1978;Punte, Rigotti, Rivero, Podjarny & Castellano, 1980). Crystals were obtained by slow evaporation from an aqueous solution.…”
mentioning
confidence: 99%
“…The six ligands around the Fe-atom are arranged in a distorted octahedral coordination like in other nitroprussides (Castellano et al, 1977;Lanfranconi et al, 1973;Manoharan and Hamilton, 1963;Punte et al, 1980). The four equatorial CN groups emerge slightly from the plane perpendicular to the Fe -NO axis by an amount of 4.3° (in average) towards the fifth CN group (see Table 2).…”
Section: Discussionmentioning
confidence: 87%