activity
20012023
most citedPrimary black hole spin in OJ287 as determined by the General Relativity centenary flare

149 citations · 1.1k across the 27 of their papers we have counts for

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Showing 2017 · astro-ph.HEShow all

5 papers · 2 filters

astro-ph.HE2017★ 81 cited

Stochastic modeling of multiwavelength variability of the classical BL Lac object OJ 287 on timescales ranging from decades to hours

A. Goyal, L. Stawarz, S. Zola +109

We present the results of our power spectral density analysis for the BL Lac object OJ\,287, utilizing the {\it Fermi}-LAT survey at high-energy -rays, {\it Swift}-XRT in X-rays…

astro-ph.HE2017★ 18 cited

Studying the accretion geometry of EXO 2030+375 at luminosities close to the propeller regime

F. Fuerst, P. Kretschmar, J. J. E. Kajava +10

The Be X-ray binary EXO 2030+375 was in an extended low luminosity state during most of 2016. We observed this state with NuSTAR and Swift, supported by INTEGRAL observations as we…

astro-ph.HE2017

EXO 2030+375 Restarts in Reverse

Peter Kretschmar, Felix Fuerst, Colleen A. Wilson-Hodge +8

The Be X-ray binary pulsar EXO 2030+375, first detected in 1985, has shown a significant detected X-ray outburst at nearly every periastron passage of its 46-day orbit for the past…

astro-ph.HE2017

Stellar Winds in Massive X-ray Binaries

Peter Kretschmar, Silvia Martínez-Núñez, Enrico Bozzo +15

Strong winds from massive stars are a topic of interest to a wide range of astrophysical fields. In High-Mass X-ray Binaries the presence of an accreting compact object on the one…

astro-ph.HE2017★ 144 cited

Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries

Silvia Martínez-Núñez, Peter Kretschmar, Enrico Bozzo +13

Massive stars, at least 10 times more massive than the Sun, have two key properties that make them the main drivers of evolution of star clusters, galaxies, and the Universe…