ALBERT

All Library Books, journals and Electronic Records Telegrafenberg

feed icon rss

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
  • 1
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Berichte der deutschen chemischen Gesellschaft 124 (1991), S. 2677-2684 
    ISSN: 0009-2940
    Keywords: Phosphaalkenes, C-halo, C-metal ; “Phospha-isonitrile” ; Phosphinylidenemethylene ; Phosphaalkyne, E/Z isomers ; Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: C-Halophosphaalkenes (1, 2) were prepared in high yield by a one-pot synthesis from HCX3 or CI4 and Mes* PCl2 (Mes* = supermesityl = 2,4,6-tri-tert-butylphenyl). The C-iodophosphaalkenes Mes* P = Cl2 (1 C) and Mes*P = CHI (2c) undergo halogen-metal exchange with n-BuLi at low temperatures. The resulting carbenoids Mes*P = CILi (11 c) and Mes*P = CHLi (6) reacted with ClMMe3 (M = Si, Ge, Sn) to give Mes*P=CIMMe3 [(Z)-13: M = Ge; (Z)-14: M = Sn] or Mes*P = CHMMe3 (8-10), respectively. Further reaction of (Z)-13 and (Z)-14 with nBuLi and ClMMe3 gave Mes*P=C(MMe3 (18: M=Ge; 19: M = Sn). The carbenoid (Z)-11 c decomposed at -85°C; instead of the expected “phosphaisonitrile” Mes*P = C : (21), only Mes*C≡P (15) was obtained which lends experimental support to the theoretically predicted instability of 21.
    Additional Material: 2 Tab.
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 2
    ISSN: 0009-2940
    Keywords: Bicyclo[1.1.0]butylcarbinyl sulfonates, solvolysis of ; Cyclobutylcarbinyl sulfonates, solvolysis of ; Anchimeric assistance in solvolysis ; Rearrangement of carbocations ; Electron demand in ditosylates ; Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Solvolyses of cis-tricyclo[3.1.0.02,6]hex-3,4-diyl ditosylate (12) and cis-bicyclo[2.1.1]hex-2,3-diyl ditosylate (27) have been carried out in 80% aqueous ethanol in the presence of ethyl-diisopropylamine. In the former case, endo,endo-tricyclo[2.2.0.02,6]hexane-3,5-diol (13a), its monoether 13b and diether 13c were products whereas in the latter the monoethers 28b, d, e, g and the diethers 28a, c, f of bicyclo[3.1.0]hexane were formed. In pure ethanol, 12 was converted into pure 13c in good yield. In the presence of the weaker base 2,6-lutidine, the solvolysis of 12 in aqueous ethanol gave different products, i.e. exo,exo-4,6-diethoxybicyclo[3.1.0]hex-2-ene (14a) and several aldehydes, inter alia cyclopentadiene-1-carboxaldehyde (15). In control experiments, the tricyclic compounds 13b, c were converted into 14a, 15 and further aldehydes as well as into the bicyclo[2.1.1]hexene derivatives 19a, b. Sulfonates of tricyclo[3.1.0.02,6]hexan-3-ol (21a) could not be isolated but its mesylate 21c was characterized by NMR spectroscopy and hydrolysed in aqueous acetone to give tricyclo[2.2.0.02,6]hexan-endo-3-ol (22a). It is concluded from these results that the dissociations of the above sulfonates do not lead to unrearranged carbocations. Rather, they proceed with participation of the β-carbon in trans position relative to the leaving group resulting in the immediate generation of rearranged cations.-Kinetic studies show that the tricyclic mesylate 21c solvolyses in 80% ethanol/water 1.4 · 105 times as fast as bicyclo[2.1.1]hex-2-yl tosylate (25), and the tricyclic ditosylate 12 solvolyses 6 · 105 as fast as the corresponding bicyclic ditosylate 27. These rate enhancements are similar to those previously observed for less strained cyclopropylcarbinyl substrates.
    Additional Material: 6 Tab.
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 3
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Berichte der deutschen chemischen Gesellschaft 124 (1991), S. 2731-2738 
    ISSN: 0009-2940
    Keywords: Bismuthinidene complexes ; Manganese complexes ; Chelating ligands ; Cumulenes ; Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Treatment of [Cp′Mn(CO)2THF] (Cp′=C5H4Me) with BiCl3 at 20°C affords the “bismuthinidene” species [Cp′- (CO)2Mn]2BiCl (1b) and very small amounts of the “star-type” compound [Cp′(CO)2Mn]3Bi2 (2). Higher yields of both compounds are obtained from the reaction of BiCl3 with [Na] [Cp′(CO)2MnSi(C6H5)3-]. The molecular structure of 1b has been determined by an X-ray diffraction study, which shows that the bismuth atom, having a trigonal-planar coordination geometry, is bonded to two manganese atoms and one chlorine atom. There are weak interactions between the molecules of 1b in the solid state thus forming infinite spiral chains of “inidene” complexes. Compound 1b reacts with NaI to afford the iodine-substituted species [Cp′(CO)2Mn]2BiI (3). Displacement of the chloride substituent from 1b by anionic chelating ligands AB- is also possible; 1b reacts with tropolonate, 8-oxoquinolate, or 8-mercaptoquinolate to form the bismuth(I) chelate compounds [CP′(CO)2Mn]Bi - AB (5a-c). The molecular structure of 5b has been determined by X-ray crystallography which shows the bismuth atom in a pseudo trigonalbipyramidal geometry with the nitrogen atom lying above the plane defined by the two manganese and the oxygen atoms in an apical position. The molecular structure of 5c has also been determined, and although the numerical values are not very accurate, the coordination geometry of the bismuth atom is seen to be intermediate between pseudo trigonalbipyramidal and distorted tetrahedral. Abstraction of a chloride ligand from 1b by Me3SiOSO2CF3 affords the cationic cumulene-type complex [Cp′(CO)2Mn=Bi=Mn(CO)2Cp][CF3SO3] (6a). Dichloromethane solutions of 6a are not stable at room temperature but may be treated with 2,-2′-bipyridine (bpy) to afford the stable adduct [{CP′(CO)2Mn}2Bi(bpy)][CF3SO3](7). The molecular structure of 7 has been determined by X-ray analysis, and - similarly to 5c, although the numerical values are not very accurate - the overall geometry has been determined unequivocally. The bismuth atom is shown to have a distorted tetrahedral geometry, thus being ligated by two manganese atoms and the two nitrogen atoms of the bpy ligands.
    Additional Material: 5 Ill.
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 4
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Zeitschrift für anorganische Chemie 400 (1973), S. 37-44 
    ISSN: 0044-2313
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Description / Table of Contents: Dehydration of Alkaline Earth Halide Hydrates in Self-generated AtmosphereThe dehydration of BaCl2 · 2 H2O, SrCl2 · 6 H2O, SrBr2 · 6 H2O, CaCl2, 6 H2O, CaCl2 · 2 H2O, and MgCl2 · 6 H2O in self-generated atmosphere was investigated by T. G. and D. T. A. methods. From the D. T. A. curves it is possible to evaluate separate melting and dehydration processes.
    Notes: Mit thermogravimetrischen und differential-thermoanalytischen Methoden wurde der Dehydratationsvorgang von BaCl2 · 2 H2O, SrCl2 · 6 H2O, SrBr2 · 6 H2O, CaCl2 · 6 H2O, CaCl2 · 2 H2O und MgCl2 · 6 H2O in eigener Gasatmosphäre untersucht. Auf Grund der in eigener Gasatmosphäre aufgenommenen DTA-Kurven lassen sich die Schmelz- und Dehydrationsvorgänge einzeln auswerten.
    Additional Material: 6 Ill.
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 5
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Zeitschrift für anorganische Chemie 394 (1972), S. 233-242 
    ISSN: 0044-2313
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Description / Table of Contents: The sorption of Cd2+-ions on freshly precipitated Al(OH)3 cannot be explained as a counterion exchange, as would be generally expected for cations. It is shown by kinetic measurements, that the process of sorption is composed of two consecutive reactions, at least one of which must be a chemisorption process. Moreover, the sorption process is controlled by a pH-dependent reaction, which previously has reached its equilibrium state.
    Notes: Die Sorption von Cd2+-Ionen an gelartigem Aluminiumhydroxid ist nicht, wie allgemein für Kationen erwartet, als counterion-exchange aufzufassen. Kinetische Messungen zeigen, daß der Sorptionsvorgang aus zwei nacheinander ablaufenden Reaktionen erster Ordnung besteht, von denen zumindest die zweite eine Chemisorption darstellt. Ein pH-abhängiges Gleichgewicht ist der Sorption vorgelagert.
    Additional Material: 4 Ill.
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 6
    Publication Date: 2017-12-22
    Description: On 17 August 2017, Swope Supernova Survey 2017a (SSS17a) was discovered as the optical counterpart of the binary neutron star gravitational wave event GW170817. We report time-series spectroscopy of SSS17a from 11.75 hours until 8.5 days after the merger. Over the first hour of observations, the ejecta rapidly expanded and cooled. Applying blackbody fits to the spectra, we measured the photosphere cooling from 11,000–900+3400 to 9300–300+300 kelvin, and determined a photospheric velocity of roughly 30% of the speed of light. The spectra of SSS17a began displaying broad features after 1.46 days and evolved qualitatively over each subsequent day, with distinct blue (early-time) and red (late-time) components. The late-time component is consistent with theoretical models of r-process–enriched neutron star ejecta, whereas the blue component requires high-velocity, lanthanide-free material.
    Keywords: Astronomy
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Geosciences , Computer Science , Medicine , Natural Sciences in General , Physics
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 7
    Publication Date: 2017-12-22
    Description: On 17 August 2017, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the Virgo interferometer detected gravitational waves (GWs) emanating from a binary neutron star merger, GW170817. Nearly simultaneously, the Fermi and INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory) telescopes detected a gamma-ray transient, GRB 170817A. At 10.9 hours after the GW trigger, we discovered a transient and fading optical source, Swope Supernova Survey 2017a (SSS17a), coincident with GW170817. SSS17a is located in NGC 4993, an S0 galaxy at a distance of 40 megaparsecs. The precise location of GW170817 provides an opportunity to probe the nature of these cataclysmic events by combining electromagnetic and GW observations.
    Keywords: Astronomy
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Geosciences , Computer Science , Medicine , Natural Sciences in General , Physics
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 8
    Publication Date: 2017-12-22
    Description: On 17 August 2017, gravitational waves (GWs) were detected from a binary neutron star merger, GW170817, along with a coincident short gamma-ray burst, GRB 170817A. An optical transient source, Swope Supernova Survey 17a (SSS17a), was subsequently identified as the counterpart of this event. We present ultraviolet, optical, and infrared light curves of SSS17a extending from 10.9 hours to 18 days postmerger. We constrain the radioactively powered transient resulting from the ejection of neutron-rich material. The fast rise of the light curves, subsequent decay, and rapid color evolution are consistent with multiple ejecta components of differing lanthanide abundance. The late-time light curve indicates that SSS17a produced at least ~0.05 solar masses of heavy elements, demonstrating that neutron star mergers play a role in rapid neutron capture (r-process) nucleosynthesis in the universe.
    Keywords: Astronomy
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Geosciences , Computer Science , Medicine , Natural Sciences in General , Physics
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 9
    Publication Date: 2018-06-08
    Description: A lightweight, rugged, high-spectral-resolution interferometer has been built by Designs and Prototypes based on a set of specifications provided by the Jet Propulsion Laboratory and Dr. J. W. Salisbury (Johns Hopkins University). The instrument, the micro Fourier Transform Interferometer (mFTIR), permits the acquisition of infrared spectra of natural surfaces. Such data can be used to validate low and high spectral resolution data acquired remotely from aircraft and spacecraft in the 3-5 mm and 8-14 mm atmospheric window. The instrument has a spectral resolutions of ~6 wavenumbers, weighs 16 kg including batteries and computer, and can be operated easily by two people in the field. Laboratory analysis indicates the instrument is spectrally calibrated to better than 1 wavenumber and the radiometric accuracy is 〈0.5 K if the radiances from the blackbodies used for calibration bracket the radiance from the sample.
    Keywords: Earth Resources and Remote Sensing
    Type: Remote Sensing of Environment
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 10
    Publication Date: 2018-06-06
    Description: The most practical way to get a spatially broad and continuous measurements of the surface temperature in the data-sparse cryosphere is by satellite remote sensing. The uncertainties in satellite-derived LSTs must be understood to develop internally-consistent decade-scale land-surface temperature (LST) records needed for climate studies. In this work we assess satellite-derived "clear-sky" LST products from the Moderate Resolution Imaging Spectroradiometer (MODIS) and the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), and LSTs derived from the Enhanced Thematic Mapper Plus (ETM+) over snow and ice on Greenland. When possible, we compare satellite-derived LSTs with in-situ air-temperature observations from Greenland Climate Network (GC-Net) automatic-weather stations (AWS). We find that MODIS, ASTER and ETM+ provide reliable and consistent LSTs under clear-sky conditions and relatively-flat terrain over snow and ice targets over a range of temperatures from -40 to 0 C. The satellite-derived LSTs agree within a relative RMS uncertainty of approx.0.5 C. The good agreement among the LSTs derived from the various satellite instruments is especially notable since different spectral channels and different retrieval algorithms are used to calculate LST from the raw satellite data. The AWS record in-situ data at a "point" while the satellite instruments record data over an area varying in size from: 57 X 57 m (ETM+), 90 X 90 m (ASTER), or to 1 X 1 km (MODIS). Surface topography and other factors contribute to variability of LST within a pixel, thus the AWS measurements may not be representative of the LST of the pixel. Without more information on the local spatial patterns of LST, the AWS LST cannot be considered valid ground truth for the satellite measurements, with RMS uncertainty approx.2 C. Despite the relatively large AWS-derived uncertainty, we find LST data are characterized by high accuracy but have uncertain absolute precision.
    Keywords: Earth Resources and Remote Sensing
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...