Tipo de publicación: Con árbitro

  • Publicación
    White Dwarfs in the UKIRT Infrared Deep Sky Survey Data Release 9
    We have identified 8 to 10 new cool white dwarfs from the Large Area Survey (LAS) Data Release 9 of the United Kingdom InfraRed Telescope (UKIRT) Infrared Deep...
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    White dwarfs with planetary remnants in the era of Gaia - I. Six emission line systems
    White dwarfs with emission lines from gaseous debris discs are among the rarest examples of planetary remnant hosts, but at the same time they are key objects...
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    Who's in the Driver's Seat: Magnetic Fields or Turbulence?
    New polarization data at 850 microns of OMC2 in Orion A are presented. These measurements trace the direction of magnetic fields in the densest parts of the...
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    Whole Earth Telescope Observations and Seismological Analysis of the Cool ZZ Ceti Star GD 154
    Fast photometric observations of a cool DAV star, GD 154, obtained with the Whole Earth Telescope are presented. GD 154 is one of the coolest pulsating DA white...
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    Whole Earth Telescope observations and seismological analysis of the cool ZZ Ceti star GD 154.
    This paper presents the results of high speed photometric observations of the cool variable DA white dwarf (DAV) GD 154 obtained with the Whole Earth Telescope...
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    Whole Earth Telescope observations of BPM 37093: A seismological test of crystallization theory in white dwarfs
    BPM 37093 is the only hydrogen-atmosphere white dwarf currently known which has sufficient mass (~1.1 M&sun;) to theoretically crystallize while still inside...
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    Whole Earth telescope observations of the ZZ Ceti star HL Tau 76
    This paper analyses the Whole Earth Telescope observations of HL Tau 76, the first discovered pulsating DA white dwarf. The star was observed during two Whole...
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    WHT follow-up observations of extremely metal-poor stars identified from SDSS and LAMOST
    Aims: We have identified several tens of extremely metal-poor star candidates from SDSS and LAMOST, which we follow up with the 4.2 m William Herschel Telescope...
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    Why Buckling Stellar Bars Weaken in Disk Galaxies
    Young stellar bars in disk galaxies experience a vertical buckling instability that terminates their growth and thickens them, resulting in a characteristic...