Tipo de publicación: Con árbitro

  • Publicación
    No evidence for a low-mass black hole in Swift J1753.5-0127
    We present high-resolution, time-resolved optical spectroscopy of the black hole X-ray transient Swift J1753.5-0127. Our optical spectra do not show features...
  • Publicación
    No evidence for black hole spin powering of jets in X-ray binaries
    In this paper, we consider the reported measurements of black hole spin for black hole X-ray binaries and compare them against the measurements of jet power and...
  • Publicación
    No Evidence for Critical Balance in Field-aligned Alfvénic Solar Wind Turbulence
    The properties of Alfvénic solar wind turbulence have been studied for decades using spacecraft measurements. In particular, the observation of spectral...
  • Publicación
    No evidence for large-scale outflows in the extended ionized halo of ULIRG Mrk273
    We present deep new Gran Telescopio Canarias (GTC) narrow-band images and William Herschel Telescope (WHT) long-slit spectroscopy of the merging system Mrk273...
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    No Evidence for Orbital Clustering in the Extreme Trans-Neptunian Objects
    The apparent clustering in longitude of perihelion ϖ and ascending node Ω of extreme trans-Neptunian objects (ETNOs) has been attributed to the gravitational...
  • Publicación
    No evidence for small disk-like bulges in a sample of late-type spirals
    Context. About 20% of low-redshift galaxies are late-type spirals with a small or no bulge component. Although they are the simplest disk galaxies in terms of...
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    No random transits in CHEOPS observations of HD 139139
    Context. The star HD 139139 (a.k.a. `the Random Transiter') is a star that exhibited enigmatic transit-like features with no apparent periodicity in K2 data...
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    No sign (yet) of intergalactic globular clusters in the Local Group
    We present Gemini Multi-Object Spectrograph (GMOS) imaging of 12 candidate intergalactic globular clusters (IGCs) in the Local Group, identified in a recent...
  • Publicación
    No Surviving Companion in Kepler's Supernova
    We have surveyed Kepler’s supernova remnant in search of the companion star of the explosion. We have gone as deep as 2.6 L ⊙ in all stars within 20% of the...