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19922026
most citedRecurrence Plots for the Analysis of Complex Systems

3.9k citations

Showing 2007Show all

51 papers · 1 filter

astro-ph2007★ 5 cited

Revised element abundances for WC-type central stars

H. Todt, G. Gräfener, W. -R. Hamann

According to previous spectral analyses of Wolf-Rayet type central stars, late [WC] subtypes show systematically higher carbon-to-helium abundance ratios than early [WC] subtypes.…

astro-ph2007

Determining element abundances of [WC]-type Central Stars for probing stellar evolution and nucleosynthesis

H. Todt, M. Peña, W. -R. Hamann +1

[WC]-type CSPNs are hydrogen-deficient Central Stars of Planetary Nebulae showing strong stellar winds and a carbon-rich chemistry. We have analyzed new high-resolution spectra of…

quant-ph2007★ 12 cited

Quantum-limited position measurements of a dark matter-wave soliton

Antonio Negretti, Carsten Henkel, Klaus Molmer

We show that the position of a dark matter-wave soliton can be determined with a precision that scales with the atomic density as . This surpasses the standard shot-noise…

astro-ph2007★ 305 cited

Non-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection

C. J. Schrijver, M. L. DeRosa, T. Metcalf +14

Solar flares and coronal mass ejections are associated with rapid changes in field connectivity and powered by the partial dissipation of electrical currents in the solar atmospher…

astro-ph2007★ 12 cited

Phase-dependent X-ray observations of the beta Lyrae system: No eclipse in the soft band

R. Ignace, L. M. Oskinova, W. L. Waldron +2

We report on observations of the eclipsing and interacting binary beta Lyrae from the Suzaku X-ray telescope. This system involves an early B star embedded in an optically and geom…

quant-ph2007

Casimir interaction between absorbing and meta Materials

F. Intravaia, C. Henkel

We investigate the Casimir energy between two dissipative mirrors in term of a sum over mode formula which can be interpreted by analogy to a quantum dissipative oscillator. We als…