Search Results - "Straal, S. M"
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HESS J1943+213: A NON-CLASSICAL HIGH-FREQUENCY-PEAKED BL LAC OBJECT
Published in The Astrophysical journal (10-05-2016)“…ABSTRACT HESS J1943+213 is an unidentified TeV source that is likely a high-frequency-peaked BL Lac (HBL) object, but that is also compatible with a pulsar…”
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X-Ray Spectroscopy of the Highly Magnetized Pulsar PSR J1846-0258, Its Wind Nebula, and Hosting Supernova Remnant Kes 75
Published in The Astrophysical journal (01-02-2021)“…Abstract We present broadband X-ray spectroscopy of the energetic components that make up the supernova remnant (SNR) Kesteven 75 using concurrent 2017 August…”
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A bright, high rotation-measure FRB that skewers the M33 halo
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT We report the detection of a bright fast radio burst, FRB 191108, with Apertif on the Westerbork Synthesis Radio Telescope. The interferometer allows…”
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X-ray Spectroscopy of the Highly Magnetized Pulsar PSR J1846-0258, its Wind Nebula and Hosting Supernova Remnant Kes 75
Published 14-09-2020“…We present broad-band X-ray spectroscopy of the energetic components that make up the supernova remnant (SNR) Kesteven 75 using concurrent 2017 Aug 17-20…”
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Apertif, Phased Array Feeds for the Westerbork Synthesis Radio Telescope
Published 30-09-2021“…A&A 658, A146 (2022) We describe the APERture Tile In Focus (Apertif) system, a phased array feed (PAF) upgrade of the Westerbork Synthesis Radio Telescope…”
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A bright, high rotation-measure FRB that skewers the M33 halo
Published 22-09-2020“…We report the detection of a bright fast radio burst, FRB\,191108, with Apertif on the Westerbork Synthesis Radio Telescope (WSRT). The interferometer allows…”
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Repeating fast radio bursts with WSRT/Apertif
Published 28-01-2020“…A&A 635, A61 (2020) Repeating fast radio bursts (FRBs) present excellent opportunities to identify FRB progenitors and host environments, as well as decipher…”
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The properties of single WO stars
Published 21-07-2014“…The enigmatic oxygen sequence Wolf-Rayet (WO) stars represent a very late stage in massive star evolution, although their exact nature is still under debate…”
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Massive stars on the verge of exploding: the properties of oxygen sequence Wolf-Rayet stars
Published 03-07-2015“…A&A 581, A110 (2015) Context. Oxygen sequence Wolf-Rayet (WO) stars represent a very rare stage in the evolution of massive stars. Their spectra show strong…”
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