Determination of sequence distributions in bacterial copolyesters containing higher alkyl and alkenyl pendant groups

1992 ◽  
Vol 25 (7) ◽  
pp. 1845-1851 ◽  
Author(s):  
Alberto Ballistreri ◽  
Giorgio Montaudo ◽  
Mario Giuffrida ◽  
Robert W. Lenz ◽  
Young B. Kim ◽  
...  
2002 ◽  
Vol 58 (3) ◽  
pp. 98-105 ◽  
Author(s):  
Wen-chuan Hsieh ◽  
Kimihiko Nishiwaki ◽  
Nobuyuki Tanaka ◽  
Hiroshi Mitomo

1971 ◽  
Vol 44 (4) ◽  
pp. 1015-1024 ◽  
Author(s):  
I. J. Gardner ◽  
C. Cozewith ◽  
G. Ver Strate

Abstract Carbon-14 labeled ethylene and propylene were used to synthesize a series of copolymers of known composition to serve as standards for copolymer analyses. Polymers with broad and narrow compositional distributions and differing sequence distributions were produced by varying the catalyst system. Solution and combustion counting techniques were used to determine sample composition and then infrared calibration curves were determined on pressed polymer films utilizing several different infrared peaks. 1. Within the ranges systematically varied neither compositional nor sequence distributions affect the peak ratios studied. 2. No isotope effects exist in the polymerizations. 3. NMR analysis yields the same results as 14C analysis. 4. Use of the 1378 cm−1 methyl band as calibrated with atactic polypropylene yields agreement with the 14C data if the average of polypropylene and copolymer results is used. 5. We amend the results previously published by our laboratory.


1988 ◽  
Vol 61 (1) ◽  
pp. 36-41 ◽  
Author(s):  
Yasuyuki Tanaka ◽  
Kazuki Nunogaki ◽  
Junichi Adachi

Abstract The sequence distribution of styrene units in cured SBR was analyzed by high-resolution GPC measurement on the ozonolysis products obtained by ozonization of finely powdered samples suspended in methylene chloride followed by reductive degradation with lithium aluminum hydride. The conversion of the ozonolysis products, which were soluble in the organic layer, approximated that of an uncured sample when 100% of the calculated amount of the ozone required to react with the double bonds in the butadiene units was used. The conversion decreased slightly as the amount of ozone was increased to 220%. The fraction of monad, diad, and triad styrene sequences which were flanked by 1,4-butadiene units, and styrene long sequences—observed at the GPC exclusion limit of 3×103—leveled off at about 100 to 150% of the required ozone. In the GPC fraction corresponding to long styrene sequences, the residual butadiene units, as measured by 1H-NMR, decreased from 77 to 47% as the ozone increased from 3.7 to 80% of the required amount. Ozonization was believed to proceed rapidly on the surface of the swollen rubber particles in the initial stage, and then it progressed gradually into the inner part upon introducing excess ozone. Cured SBR samples, with and without carbon filler, showed sequence distributions of the styrene units which were similar to the uncured sample when 130% of ozone was used.


1978 ◽  
Vol 51 (2) ◽  
pp. 168-179 ◽  
Author(s):  
Yasuyuki Tanaka ◽  
Hisaya Sato ◽  
Koichi Hatada ◽  
Yoshio Teeawaki ◽  
Hiroshi Okuda

Abstract The spin-decoupled 1H NMR and 13C NMR methods were employed for the determination of the cis-trans sequence distribution in polybutadiene. Poly(butadiene-2,3-d2) and cis-trans isomerized polybutadienes were used for the peak assignment and the resonance of methylene protons in cis-trans linkage could be described as an A1B2 system. The dyad and triad sequence distributions of cis-1,4 and trans-1,4 units were determined for isomerized, equibinary, and lithium catalyzed polybutadienes, and polycyclooctadienes. The accuracy of the measurements was also studied comparing the results with those by infrared method.


1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.


1961 ◽  
Vol 13 ◽  
pp. 29-41
Author(s):  
Wm. Markowitz
Keyword(s):  

A symposium on the future of the International Latitude Service (I. L. S.) is to be held in Helsinki in July 1960. My report for the symposium consists of two parts. Part I, denoded (Mk I) was published [1] earlier in 1960 under the title “Latitude and Longitude, and the Secular Motion of the Pole”. Part II is the present paper, denoded (Mk II).


1972 ◽  
Vol 1 ◽  
pp. 27-38
Author(s):  
J. Hers

In South Africa the modern outlook towards time may be said to have started in 1948. Both the two major observatories, The Royal Observatory in Cape Town and the Union Observatory (now known as the Republic Observatory) in Johannesburg had, of course, been involved in the astronomical determination of time almost from their inception, and the Johannesburg Observatory has been responsible for the official time of South Africa since 1908. However the pendulum clocks then in use could not be relied on to provide an accuracy better than about 1/10 second, which was of the same order as that of the astronomical observations. It is doubtful if much use was made of even this limited accuracy outside the two observatories, and although there may – occasionally have been a demand for more accurate time, it was certainly not voiced.


Sign in / Sign up

Export Citation Format

Share Document