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Encoding Disappearing Characters: The Case of Twentieth-Century Japanese-Canadian Names
Published 2019-08-01Subjects: Get full text
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ALMA Observations of Solar Spicules in a Polar Coronal Hole
Published 2025-01-01“…\limits^{\unicode{x02033}}$ 5 × 0 $\mathop{.}\limits^{\unicode{x02033}}$ 7, respectively. …”
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Identifier syntax and mnemonics in programming languages
Published 2000-12-01“…Unicode itself provides syntax rules for identifiers, in order to ensure uniform treatment of identifiers. …”
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Testing the Flux Rope Paradigm for Coronal Mass Ejections Using a Three-spacecraft Encounter Event
Published 2025-01-01“…\limits^{\unicode{x000b0}}$ 7 east of Earth. The reconstruction assumes a magnetic flux rope (MFR) structure for the CME. …”
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Envejecimiento poblacional: actualidad y futuro
Published 2017-02-01“…<p class="western" style="margin-bottom: 0cm; font-weight: normal; line-height: 150%;" align="JUSTIFY"><span style="font-family: DejaVu Sans Condensed,Arial Unicode MS,sans-serif;"><br /></span></p>…”
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First fluctuation measurements using an Imaging Neutral Particle Analyzer on DIII-D
Published 2025-01-01“…Simulated measurements in the range of pitches that the diagnostic is sensitive to ( $0.5\unicode{x2A7D} \left| \frac{v_{\parallel}}{v} \right| \unicode{x2A7D} 0.75$ ) show the signal is dominated by trapped orbits that pass through magnetic islands near the edge of the plasma. …”
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Projet urbain et paysage littoral
Published 2009-06-01“…The objective was to take the « landscape» out of the discourse relating to the « beauty», to develop a methodological frame renewing the local monograph in order to analyze the scale unicode2utf8(0x2018)from the local to the global». …”
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Search for Neutrino Signals Correlated with LHAASO Diffuse Galactic Emission
Published 2025-01-01“…In the Galactic plane scan search, the most significant location is found at l = 63 $\mathop{.}\limits^{\unicode{x000B0}}$ 57 and b = 0 $\mathop{.}\limits^{\unicode{x000B0}}$ 93 with a pretrial (posttrial) significance of 4.6 σ (1.8 σ ).…”
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Elevated Rates of Tidal Disruption Events in Active Galactic Nuclei
Published 2025-01-01“…For M _• ~ 10 ^7 M _⊙ and M _d ~ 0.1 M _• , the rate enhancement can be up to a factor ${\dot{N}}_{{\rm{cl}}}/{\dot{N}}_{{\rm{2b}}}\unicode{x0007E}10$ . The orbits of collisionless TDEs sometimes have a preferred orientation in apses, carrying implications for observational signatures of resulting flares.…”
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Finding Lensed Radio Sources with the Very Large Array Sky Survey
Published 2025-01-01“…We obtain high-resolution (0 $\mathop{.}\limits^{\unicode{x02033}}$ 2) VLA follow-up observations for 11 targets that we identify using three different techniques: (i) a search for compact radio sources offset from galaxies with high lensing potential, (ii) VLASS detections of known lensed galaxies, and (iii) VLASS detections of known lensed quasars. …”
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Pushing the Atacama Large Millimeter/submillimeter Array to the Limit: 140 pc Resolution Observations of a z = 6.6 Quasar–Galaxy Merger Resolve Strikingly Different Morphologies of...
Published 2025-01-01“…We find that dust continuum is emitted in regions of $\unicode{x0007E}0^{\prime\prime} \,.02-0^{\prime\prime} \,.04$ consistent with the size of photodissociation regions (PDRs), whereas 50% of the [C ii ] originates from larger physical scales ( θ ≳ 2″). …”
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Asymmetries and Circumstellar Interaction in the Type II SN 2024bch
Published 2025-01-01“…Comparisons between models and the early spectra suggest a pre-SN mass-loss rate of $\dot{M}\,\unicode{x0007E}\,1{0}^{-3}\unicode{8210}1{0}^{-2}\,{M}_{\odot }\,{\mathrm{yr}}^{-1}$ , which is too high to be explained by quiescent mass loss from RSGs, but is consistent with some recent measurements of similar SNe. …”
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GD-1 Stellar Stream and Cocoon in the DESI Early Data Release
Published 2025-01-01“…\limits^{\unicode{x000b0}}$ 353 ∼ 55 pc) and colder [( σ = 3.09 ± 0.76 km s ^−1 )] thin stream component (based on a median per star velocity precision of 2.7 km s ^−1 ). …”
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MINDS. JWST-MIRI Observations of a Spatially Resolved Atomic Jet and Polychromatic Molecular Wind toward SY Cha
Published 2025-01-01“…This is one of the first polychromatic detections of extended H _2 toward a moderately inclined, i = 51 $\mathop{.}\limits^{\unicode{x000B0}}$ 1, Class II source. We measure the semiopening angle of the H _2 emission and build a rotation diagram to determine the H _2 excitation temperature and abundance. …”
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