output
20022026
most citedRecurrence Plots for the Analysis of Complex Systems

3.9k citations

Showing 2015Show all

29 papers · 1 filter

cond-mat.stat-mech2015★ 18 cited

Fluctuation relations for anomalous dynamics generated by time-fractional Fokker-Planck equations

P. Dieterich, R. Klages, A. V. Chechkin

Anomalous dynamics characterized by non-Gaussian probability distributions (PDFs) and/or temporal long-range correlations can cause subtle modifications of conventional fluctuation…

astro-ph.SR2015★ 122 cited

Wolf-Rayet stars in the Small Magellanic Cloud: I. Analysis of the single WN stars

R. Hainich, D. Pasemann, H. Todt +3

Wolf-Rayet (WR) stars have a severe impact on their environments owing to their strong ionizing radiation fields and powerful stellar winds. Since these winds are considered to be…

q-bio.QM2015★ 2 cited

Real sequence effects on the search dynamics of transcription factors on DNA

Maximilian Bauer, Emil S. Rasmussen, Michael A. Lomholt +1

Recent experiments show that transcription factors (TFs) indeed use the facilitated diffusion mechanism to locate their target sequences on DNA in living bacteria cells: TFs altern…

astro-ph.SR2015★ 74 cited

New near-infrared period-luminosity-metallicity relations for RR Lyrae stars and the outlook for Gaia

Tatiana Muraveva, Max Palmer, Gisella Clementini +6

We present results of the analysis of 70 RR Lyrae stars located in the bar of the Large Magellanic Cloud (LMC). Combining spectroscopically determined metallicity of these stars fr…

astro-ph.SR2015★ 25 cited

B fields in OB stars (BOB): FORS2 spectropolarimetric follow-up of the two rare rigidly rotating magnetosphere stars HD23478 and HD345439

S. Hubrig, M. Schöller, L. Fossati +7

Massive B-type stars with strong magnetic fields and fast rotation are very rare and provide a mystery for theories of both star formation and magnetic field evolution. Only two su…

astro-ph.SR2015★ 18 cited

The donor star of the X-ray pulsar X1908+075

Silvia Martínez-Núñez, Andreas Sander, Ángel Gímenez-García +4

High-mass X-ray binaries (HMXBs) consist of a massive donor star and a compact object. While several of those systems have been well studied in X-rays, little is known for most of…