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  • The origin of pulsating ult... The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors
    Misra, D.; Fragos, T.; Tauris, T. M. ... Astronomy & astrophysics, 10/2020, Volume: 642
    Journal Article
    Peer reviewed
    Open access

    Context. Ultra-luminous X-ray sources (ULXs) are those X-ray sources located away from the centre of their host galaxy with luminosities exceeding the Eddington limit of a stellar-mass black hole ( L ...
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2.
  • Predictions for the hydroge... Predictions for the hydrogen-free ejecta of pulsational pair-instability supernovae
    Renzo, M.; Farmer, R.; Justham, S. ... Astronomy & astrophysics, 08/2020, Volume: 640
    Journal Article
    Peer reviewed
    Open access

    Present and upcoming time-domain astronomy efforts, in part driven by gravitational-wave follow-up campaigns, will unveil a variety of rare explosive transients in the sky. Here, we focus on ...
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3.
  • Spectral models for binary ... Spectral models for binary products: Unifying subdwarfs and Wolf-Rayet stars as a sequence of stripped-envelope stars
    Götberg, Y.; de Mink, S. E.; Groh, J. H. ... Astronomy & astrophysics, 07/2018, Volume: 615
    Journal Article
    Peer reviewed
    Open access

    Stars stripped of their hydrogen-rich envelope through interaction with a binary companion are generally not considered when accounting for ionizing radiation from stellar populations, despite the ...
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4.
  • Contribution from stars str... Contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium
    Götberg, Y.; de Mink, S. E.; McQuinn, M. ... Astronomy & astrophysics, 02/2020, Volume: 634
    Journal Article
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    Open access

    Massive stars are often found in binary systems, and it has been argued that binary products boost the ionizing radiation of stellar populations. Accurate predictions for binary products are needed ...
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5.
  • Effect of binary evolution ... Effect of binary evolution on the inferred initial and final core masses of hydrogen-rich, Type II supernova progenitors
    Zapartas, E.; de Mink, S. E.; Justham, S. ... Astronomy & astrophysics, 01/2021, Volume: 645
    Journal Article
    Peer reviewed
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    The majority of massive stars, which are the progenitors of core-collapse supernovae (SNe), are found in close binary systems. In a previous work, we modeled the fraction of hydrogen-rich, Type II SN ...
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6.
  • Clues about the scarcity of... Clues about the scarcity of stripped-envelope stars from the evolutionary state of the sdO+Be binary system φ Persei
    Schootemeijer, A.; Götberg, Y.; de Mink, S. E. ... Astronomy & astrophysics, 07/2018, Volume: 615
    Journal Article
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    Stripped-envelope stars form in binary systems after losing mass through Roche-lobe overflow. They bear astrophysical significance as sources of UV and ionizing radiation in older stellar populations ...
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7.
  • Delay-time distribution of ... Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction
    Zapartas, E.; de Mink, S. E.; Izzard, R. G. ... Astronomy & astrophysics, 05/2017, Volume: 601
    Journal Article
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    Most massive stars, the progenitors of core-collapse supernovae, are in close binary systems and may interact with their companion through mass transfer or merging. We undertake a population ...
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8.
  • Rejuvenated Accretors Have ... Rejuvenated Accretors Have Less Bound Envelopes: Impact of Roche Lobe Overflow on Subsequent Common Envelope Events
    Renzo, M.; Zapartas, E.; Justham, S. ... Astrophysical journal. Letters, 01/2023, Volume: 942, Issue: 2
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    Abstract Common envelope (CE) evolution is an outstanding open problem in stellar evolution, critical to the formation of compact binaries including gravitational-wave sources. In the “classical” ...
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  • Predicting the Presence of ... Predicting the Presence of Companions for Stripped-envelope Supernovae: The Case of the Broad-lined Type Ic SN 2002ap
    Zapartas, E.; Mink, S. E. de; Dyk, S. D. Van ... Astrophysical journal/˜The œAstrophysical journal, 06/2017, Volume: 842, Issue: 2
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    Many young, massive stars are found in close binaries. Using population synthesis simulations we predict the likelihood of a companion star being present when these massive stars end their lives as ...
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10.
  • Ejection of the Massive Hyd... Ejection of the Massive Hydrogen-rich Envelope Timed with the Collapse of the Stripped SN 2014C
    Margutti, Raffaella; Kamble, A.; Milisavljevic, D. ... Astrophysical journal/˜The œAstrophysical journal, 02/2017, Volume: 835, Issue: 2
    Journal Article
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    We present multi-wavelength observations of SN 2014C during the first 500 days. These observations represent the first solid detection of a young extragalactic stripped-envelope SN out to high-energy ...
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