Na 1 Nachlass Max Horkheimer, 44 - Korrespondenzen u.a. mit Marthe Roth (p. I 21, 313-463)

2 Briefe und 1 Lebenslauf von Max Horkheimer an Arthur Rosenberg, 1939, 1941; 2 Briefe zwischen Kurt Rosenfeld und Karl Brandt, 22.04.1937, 27.04.1937; 5 Briefe von Kurt Rosenfeld an Max Horkheimer, 1937-19378; 4 Brief und Beilage an Kurt Rosenfeld, 1937-1943; 11 Briefe zwischen Hans W. Rosenhaupt und Max Horkheimer, 1935, 1941, 1942, 1947; 4 Briefe zwischen Samuel I. Roseman und Max Horkheimer, 1939, 03.01.1940; 2 Briefe zwischen J. Rosenstock und Max Horkheimer, 15.07.1946; 2 Briefe zwischen Joseph Adolphe Rosenthal und Max Horkheimer, 09.04.1941, 08.05.1941, sowie Briefwechsel mit Sophie Ries; 2 Briefe zwischen Sophie Ries und Max Horkheimer, 08.05.1941, 11.05.1941; 1 Brief von Max Horkheimer an Lore Woedthke, 08.05.1941; 2 Briefe zwischen Morris Rosenthal und Max Horkheimer, 01.10.1935, 04.10.1935; 1 Brief von Max Horkheimer an das Rosenwald Capital Outlay Fund New York, 30.01.1940; 1 Brief B. Lifschitz an Marthe Roth, 21.04.1937; 1 Brief von Chamorel et Simond an Marthe Roth, 11.06.1937; 1 Brief von F.K. Sung an Marthe Roth, 24.06.1937; 12 Briefe zwischen Marthe Roth und Max Horkheimer, Juli 1937-1938, sowie Briefwechsel mit Louis Vogt; 4 Briefe zwischen Louis Vogt und Max Horkheimer, 10.08.1937, 1937; 1 Brief von Max Horkheimer an Dr. Rothen, 31.01.1935; 1 Umzugsmitteilung von Hans Rothmann; 2 Briefe zwischen Richard C. Rothschild und Max Horkheimer, 11.05.1940, 13.05.1940; 4 Briefe zwischen Ludwig Rothschild, Hilde Rothschild und Max Horkheimer, 1936-15.09.1939; 2 Briefe zwischen S. Rothschildt und Max Horkheimer, 23.11.1940, 29.11.1940; 4 Brief zwischen J. S. Roucek und Max Horkheimer, 1941; 1 Brief von Joseph Rovan an Max Horkheimer, 11.05.1948; 2 Brief zwischen Wilmina Rowland und Max Horkheimer, 13.03.1949, 11.04.1949; 2 Briefe zwischen dem Royal Automobile Club und Max Horkheimer, 26.08.1937, 22.09.1937; 2 Briefe zwischen Royal Motors Inc. und Max Horkheimer, 05.02.1940, 06.03.1940; 1 Beitrag von Nina Rubinstein zur Soziologie des Fremden; 1 Brief von Theodor W. Adorno an Rudd, 09.09.1940; 1 Brief von Jay Rumney an Goldstein, 18.06.1936; 20 Briefe und Beilage zwischen Jay Rumney und Max Horkheimer, 1934- 1937, 1949 sowie Briefwechsel mit D. Mitrany; 3 Briefe zwischen D. Mitrany und Max Horkheimer, 01.12.1937, 1937; 3 Briefe von Theodor W. Adorno an Dagobert D. Runes, 1941; 1 Brief und 1 Beilage von N. Waterman an Georg Rusche, 03.05.1939; 12 Briefe und Beilage zwischen Georg Rusche und Max Horkheimer, 1939-1942 sowie Briefwechsel mit N. Waterman; 1 Brief von N. Waterman an Georg Rusche, 03.04.1939; 2 Briefe zwischen N. Waterman und Max Horkheimer, 21.04.1939, 05.05.1939; 1 Brief von Ruth an Max Horkheimer;

GRO J1008−57: an (almost) predictable transient X-ray binary

A study of archival RXTE, Swift, and Suzaku pointed observations of the transient high-mass X-ray binary GRO J1008−57 is presented. A new orbital ephemeris based on pulse arrival-timing shows the times of maximum luminosities during outbursts of GRO J1008−57 to be close to periastron at orbital phase − 0.03. This makes the source one of a few for which outburst dates can be predicted with very high precision. Spectra of the source in 2005, 2007, and 2011 can be well described by a simple power law with high-energy cutoff and an additional black body at lower energies. The photon index of the power law and the black-body flux only depend on the 15–50 keV source flux. No apparent hysteresis effects are seen. These correlations allow us to predict the evolution of the pulsar’s X-ray spectral shape over all outbursts as a function of just one parameter, the source’s flux. If modified by an additional soft component, this prediction even holds during GRO J1008−57’s 2012 type II outburst.

No anticorrelation between cyclotron line energy and X-ray flux in 4U 0115+634

We report on an outburst of the high mass X-ray binary 4U 0115+634 with a pulse period of 3.6 s in 2008 March/April as observed with RXTE and INTEGRAL. During the outburst the neutron star’s luminosity varied by a factor of 10 in the 3–50 keV band. In agreement with earlier work we find evidence of five cyclotron resonance scattering features at ~10.7, 21.8, 35.5, 46.7, and 59.7 keV. Previous work had found an anticorrelation between the fundamental cyclotron line energy and the X-ray flux. We show that this apparent anticorrelation is probably due to the unphysical interplay of parameters of the cyclotron line with the continuum models used previously, e.g., the negative and positive exponent power law (NPEX). For this model, we show that cyclotron line modeling erroneously leads to describing part of the exponential cutoff and the continuum variability, and not the cyclotron lines. When the X-ray continuum is modeled with a simple exponentially cutoff power law modified by a Gaussian emission feature around 10 keV, the correlation between the line energy and the flux vanishes, and the line parameters remain virtually constant over the outburst. We therefore conclude that the previously reported anticorrelation is an artifact of the assumptions adopted in the modeling of the continuum.

Luminosity dependent accretion state change in GRO J1008–57

In a former publication, we have analyzed the transient neutron star X-ray binary GRO J1008–57 using all available RXTE-, Swift-, and Suzaku-data. As we have found, the source’s spectral components, i.e., a power-law with high exponential cutoff and a black-body, are strongly correlated with the hard X-ray flux (15–50 keV). We update the analytical description of these dependence, including a change in the photon index behaviour from a flat to a logarithmic function. The flux, where the change occurs, is consistent with the onset of the black-body emission. Thus, a change of the accretion state always occurs in GRO J1008–57 at a particular flux level.

The Goodness of Simultaneous Fits in ISIS

In a previous work, we introduced a tool for analyzing multiple datasets simultaneously, which has been implemented into ISIS. This tool was used to fit many spectra of X-ray binaries. However, the large number of degrees of freedom and individual datasets raise an issue about a good measure for a simultaneous fit quality. We present three ways to check the goodness of these fits: we investigate the goodness of each fit in all datasets, we define a combined goodness exploiting the logical structure of a simultaneous fit, and we stack the fit residuals of all datasets to detect weak features. These tools are applied to all RXTE-spectra from GRO 1008−57, revealing calibration features that are not detected significantly in any single spectrum. Stacking the residuals from the best-fit model for the Vela X-1 and XTE J1859+083 data evidences fluorescent emission lines that would have gone undetected otherwise.

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Mode of access: Internet.

Die Fugger, Rothschild, Krupp

von Richard Ehrenberg

Si vous n'avez rien à me dire : Und hast du mir kein Wort zu sagen? Frei nach V. Hugo von Richard Genée. Lied für eine Singstimme mit Begl. de. Pianoforte ; Op. 5 no. 1

von ... W. von Rothschild

Repeated blood pressure measurements in a sample of Swedish twins: heritabilities and associations with polymorphisms in the renin-angiotensin-aldosterone system Iliadou, Anastasia, Lichtenstein, Paul, Morgenstern, Ralf, Forsberg, Lena, Svensson, Richard, de Faire, Ulf, Martin, Nicholas, Pedersen, Nancy

Background Twin and family studies have shown that genetic effects explain a relatively high amount of the phenotypic variation in blood pressure. However, many studies have not been able to replicate findings of association between specific polymorphisms and diastolic and systolic blood pressure. Methods In a structural equation-modelling framework the authors investigated longitudinal changes in repeated measures of blood pressures in a sample of 298 like-sexed twin pairs from the population-based Swedish Twin Registry. Also examined was the association between blood pressure and polymorphisms in the angiotensin-I converting enzyme and the angiotensin 11 receptor type 1 with the 'Fulker' test Both linkage and association were tested simultaneously revealing whether the polymorphism is a Quantitative Trait Locus (QTL) or in linkage disequilibrium with the QTL. Results Genetic influences explained up to 46% of the phenotypic variance in diastolic and 63% of the phenotypic variance in systolic blood pressure. Genetic influences were stable over time and contributed up to 78% of the phenotypic correlation in both diastolic and systolic blood pressure. Non-shared environmental effects were characterised by time specific influences and little transmission from one time point to the next. There was no significant linkage and association between the polymorphisms and blood pressure. Conclusions There is a considerable genetic stability in both diastolic and systolic blood pressure for a 6-year period of time in adult life. Non-shared environmental influences have a small long-term effect Although associations with the polymorphisms could not be replicated, results should be interpreted with caution due to power considerations. (C) 2002 Lippincott Williams Wilkins.

O Barão de Rothschild e a questão do Acre

O autor reconstitui a criação do estado brasileiro do Acre, ressaltando os interesses estrangeiros subjacentes à disputa com a Bolívia. O protocolo pelo qual a Bolívia arrendava o território ao Bolivian Syndicate e a disposição de Rio Branco em reivindicar aquela região para o Brasil colocavam os dois países em rota de colisão. Nesse contexto surge a figura dúbia do Barão de Rothschild que propõe uma solução pacífica para o dissídio através do arbitramento da Grã Bretanha.