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zadetkov: 353
1.
  • THE IMPACT OF A SUPERNOVA R... THE IMPACT OF A SUPERNOVA REMNANT ON FAST RADIO BURSTS
    Piro, Anthony L. Astrophysical journal. Letters, 06/2016, Letnik: 824, Številka: 2
    Journal Article
    Recenzirano
    Odprti dostop

    ABSTRACT Fast radio bursts (FRBs) are millisecond bursts of radio radiation whose progenitors, so far, remain mysterious. Nevertheless, the timescales and energetics of these events have lead to many ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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2.
  • Implications from ASKAP Fas... Implications from ASKAP Fast Radio Burst Statistics
    Lu, Wenbin; Piro, Anthony L. Astrophysical journal/˜The œAstrophysical journal, 09/2019, Letnik: 883, Številka: 1
    Journal Article
    Recenzirano
    Odprti dostop

    Although there has recently been tremendous progress in studies of fast radio bursts (FRBs), the nature of their progenitors remains a mystery. We study the fluence and dispersion measure (DM) ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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3.
  • Slowing the spins of stella... Slowing the spins of stellar cores
    Fuller, Jim; Piro, Anthony L; Jermyn, Adam S Monthly notices of the Royal Astronomical Society, 05/2019, Letnik: 485, Številka: 3
    Journal Article
    Recenzirano

    ABSTRACT The angular momentum (AM) evolution of stellar interiors, along with the resulting rotation rates of stellar remnants, remains poorly understood. Asteroseismic measurements of red giant ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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4.
  • Unifying Type II Supernova ... Unifying Type II Supernova Light Curves with Dense Circumstellar Material
    Morozova, Viktoriya; Piro, Anthony L.; Valenti, Stefano Astrophysical journal/˜The œAstrophysical journal, 03/2017, Letnik: 838, Številka: 1
    Journal Article
    Recenzirano
    Odprti dostop

    A longstanding problem in the study of supernovae (SNe) has been the relationship between the Type IIP and Type IIL subclasses. Whether they come from distinct progenitors or they are from similar ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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5.
  • Measuring the Progenitor Ma... Measuring the Progenitor Masses and Dense Circumstellar Material of Type II Supernovae
    Morozova, Viktoriya; Piro, Anthony L.; Valenti, Stefano Astrophysical journal/˜The œAstrophysical journal, 05/2018, Letnik: 858, Številka: 1
    Journal Article
    Recenzirano
    Odprti dostop

    Recent modeling of hydrogen-rich Type II supernova (SN II) light curves suggests the presence of dense circumstellar material (CSM) surrounding the exploding progenitor stars. This has important ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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6.
  • Wind-reprocessed Transients Wind-reprocessed Transients
    Piro, Anthony L.; Lu, Wenbin Astrophysical journal/˜The œAstrophysical journal, 05/2020, Letnik: 894, Številka: 1
    Journal Article
    Recenzirano
    Odprti dostop

    We consider the situation where the luminosity from a transient event is reprocessed by an optically thick wind. Potential applications are the tidal disruption of stars by black holes (BHs), ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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7.
  • Optical and X-ray emission ... Optical and X-ray emission from stable millisecond magnetars formed from the merger of binary neutron stars
    Metzger, Brian D.; Piro, Anthony L. Monthly notices of the Royal Astronomical Society, 04/2014, Letnik: 439, Številka: 4
    Journal Article
    Recenzirano
    Odprti dostop

    The coalescence of binary neutron stars (NSs) may in some cases produce a stable massive NS remnant rather than a black hole. Due to the substantial angular momentum from the binary, such a remnant ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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8.
  • Evidence for Cocoon Emissio... Evidence for Cocoon Emission from the Early Light Curve of SSS17a
    Piro, Anthony L.; Kollmeier, Juna A. Astrophysical journal/˜The œAstrophysical journal, 03/2018, Letnik: 855, Številka: 2
    Journal Article
    Recenzirano
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    Swope Supernova Survey 2017a (SSS17a) was discovered as the first optical counterpart to the gravitational wave event GW170817. Although its light curve on the timescale of weeks roughly matches the ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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9.
  • WHAT CAN WE LEARN FROM THE ... WHAT CAN WE LEARN FROM THE RISING LIGHT CURVES OF RADIOACTIVELY POWERED SUPERNOVAE?
    Piro, Anthony L; Nakar, Ehud Astrophysical journal/˜The œAstrophysical journal, 05/2013, Letnik: 769, Številka: 1
    Journal Article
    Recenzirano
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    The light curve of the explosion of a star with a radius #10-100 R# is powered mostly by radioactive decay. Observationally, such events are dominated by hydrogen-deficient progenitors and classified ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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10.
  • MAGNETIC INTERACTIONS IN CO... MAGNETIC INTERACTIONS IN COALESCING NEUTRON STAR BINARIES
    PIRO, Anthony L Astrophysical journal/˜The œAstrophysical journal, 08/2012, Letnik: 755, Številka: 1
    Journal Article
    Recenzirano
    Odprti dostop

    It is expected on both evolutionary and empirical grounds that many merging neutron star (NS) binaries are composed of a highly magnetized NS in orbit with a relatively low magnetic field NS. I study ...
Celotno besedilo
Dostopno za: NUK, UL, UM, UPUK

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zadetkov: 353

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