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On the Formation of Planets in the Milky Way’s Thick Disk
Published 2025-01-01“…Exoplanet demographic surveys have revealed that close-in (≲1 au) small planets orbiting stars in the Milky Way’s thick disk are ∼50% less abundant than those orbiting stars in the Galactic thin disk. …”
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A Candidate High-velocity Exoplanet System in the Galactic Bulge
Published 2025-01-01“…The combination of the host star brightness and light curve parameters yields host star and planet masses of M _host = 0.19 ± 0.03 M _⊙ and m _p = 28.92 ± 4.75 M _⊕ at a distance of D _L = 7.49 ± 0.91 kpc. …”
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The First Galaxies and the Likely Discovery of Their Fossils in the Local Group
Published 2010-01-01“…It is widely believed that reionization stopped star formation in fossil dwarfs. However, here we dispute this idea and discuss a physical mechanism whereby recent episodes of star formation would be produced in some fossil dwarfs that, hence, may characterized by a bimodal star formation history. …”
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504
The Influence of General Relativity on the Spins of Celestial Bodies in Inclined Orbits
Published 2025-01-01“…The high obliquity observed in these planets can be attributed to two primary formation mechanisms, as summarized in the existing literature. First, the host star's spin becomes misaligned with the planetary disk during the late stages of star formation, primarily due to chaotic accretion and magnetic interactions between the star and the planetary disk. …”
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505
It takes a ‘spark’. Exploring parent perception of long-term sports participation after a practitioner-led, peer-group sports intervention for ambulant, school-aged children with c...
Published 2025-06-01“…Since attending Sports Stars, children participated in a variety of sports, the most common being swimming and soccer. …”
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506
Bulge Oscillation Driven by Outflows of Active Galactic Nuclei. I. Fast Outflow Case
Published 2025-01-01“…There is growing evidence for star formation inside outflows of active galactic nuclei (AGNs). …”
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Ratio de oxígeno como determinante de severidad en neumonía COVID-19
Published 2023-10-01Get full text
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Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3
Published 2023-03-01“…Using both binary neutron star and neutron star–black hole binaries, we obtain a broad, relatively flat neutron star mass distribution extending from 1.2_{-0.2}^{+0.1} to 2.0_{-0.3}^{+0.3}M_{⊙}. …”
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511
The Appearance and Disappearance of Exocomet Gas Absorption
Published 2015-01-01“…CaII K-line (3933 Å) absorption profiles observed towards 15 A-type and two B-type stars with known (or suspected) debris disks, in addition to archival spectral data for three A-type stars, are presented. …”
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The Effect of Galaxy Interactions on Starbursts in Milky Way-mass Galaxies in FIRE Simulations
Published 2025-01-01“…Simulations and observations suggest that galaxy interactions may enhance the star formation rate (SFR) in merging galaxies. One proposed mechanism is the torque exerted on the gas and stars in the larger galaxy by the smaller galaxy. …”
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Strangeness in Astrophysics
Published 2025-01-01“…In this contribution the role of strangeness in astrophysics is discussed and, more precisely, strange hadronic matter in the interior of neutron stars. A special attention is payed to certain phenomena involving strange hadronic matter, such as the hyperon puzzle, kaon condensation and the thermal behaviour of hyperons in neutron star mergers.…”
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Formation of SS316L Single Tracks in Micro Selective Laser Melting: Surface, Geometry, and Defects
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3D Finite Element Modeling and Modal Analysis of Planetary Gear System with Herringbone Gears
Published 2022-09-01“…A herringbone gear transmission system with star gear train is taken as the research object. …”
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Pt/IrO x enables selective electrochemical C-H chlorination at high current
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