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Urgensi Filsafat dalam Ilmu Falak dan Relevansinya bagi Kehidupan Beragama Masyarakat
Published 2020-10-01“…The findings suggest that philosophy has prominent roles for science since in astronomy, the origins of universe formation such as nebula and the big bang theory are also discussed. …”
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342
Iron-Nickel Microparticles in the Sedimentary Rocks as Indicators of Cosmic Processes
Published 2015-09-01“…It was found that the microspheres developed as a result of the fractional condensation of a Fe-Ni melt and its crystallization at the early stage of the evolution of the substance of the protosolar nebula. Upon reaching the atmosphere of the Earth, these microspheres undergo changes in terms of partial oxidation of magnetite to hematite and native nickel to nickel oxides, melting of fusible metals in the core part, and atmospheric entry under the influence of the “pulverization effect” resulting in the development of awaruite microparticles of various shapes. …”
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343
Joint photon-electron Lorentz violation parameter plane from LHAASO data
Published 2022-12-01“…By adopting the synchrotion self-Compton model, LHAASO also suggests that the 1.12PeV high-energy photon from Crab Nebula corresponds to a 2.3PeV high-energy electron. …”
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344
Discovery of an Extended γ-Ray Emission around the Supernova Remnant Candidate Associated with PSR J0837–2454
Published 2023-01-01“…Several scenarios, such as an SNR, pulsar wind nebula, and pulsar halo, are discussed as the potential origins of the extended γ -ray emission, and our model fitting results are preferred for the SNR scenario.…”
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345
Latency and resource consumption analysis for serverless edge analytics
Published 2023-07-01Get full text
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346
« Mourir dans un baiser » Un archétype du féminicide ?
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347
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TIMING AND INTERSTELLAR SCATTERING OF 35 DISTANT PULSARS DISCOVERED IN THE PALFA SURVEY
Published 2015“…Finally, we present XMM-Newton and Chandra observations of the youngest and most energetic of the pulsars, J1856+0245, which has previously been associated with the GeV-TeV pulsar wind nebula HESS J1857+026.…”
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350
D/H Ratios on Saturn and Jupiter from Cassini CIRS
Published 2017“…The Saturn D/H value is consistent with estimates for hydrogen in the protosolar nebula (2.1 ± 0.5) <strong>×</strong>10<sup>−5</sup>, but its apparent divergence from the Jovian value suggests that our understanding of planetary formation and evolution is incomplete, which is in agreement with previous work.…”
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351
Chondrule sizes within the CM carbonaceous chondrites and measurement methodologies
Published 2024“…The sizes of chondrules are a valuable tool for understanding relationships between meteorite groups and the affinity of ungrouped chondrites, documenting temporal/spatial variability in the solar nebula, and exploring the effects of parent body processing. …”
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352
JWST Reveals Powerful Feedback from Radio Jets in a Massive Galaxy at z = 4.1
Published 2024“…The outflowing gas shows velocities exceeding 900 km s−1 and broad line profiles with widths exceeding 1200 km s−1 located at an ∼10 kpc projected distance from the central nucleus. The outflowing nebula spatially overlaps with the brightest radio lobe, indicating that the powerful radio jets are responsible for the outflow kinematics. …”
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353
AN INFRARED STUDY OF THE REMARKABLE DUSTY M-STAR HR-3126
Published 1993“…HR 3126 is a unique M giant star embedded in the bipolar reflection nebula IC 2220. Its evolutionary status is uncertain, and both the composition of the dust shell and the mechanism responsible for its ejection have proved controversial. …”
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Redshift Evolution of Electron Density in the Interstellar Medium at z ∼ 0–9 Uncovered with JWST/NIRSpec Spectra and Line-spread Function Determinations
Published 2023-01-01“…The p ∼ 1−2 evolutionary relation can be explained by a combination of the compact morphology and the reduction of n _e due to the high electron temperature of high- z metal-poor nebulae.…”
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356
Constraints on the Persistent Radio Source Associated with FRB 20190520B Using the European VLBI Network
Published 2023-01-01“…We discuss the model of a magnetar in a wind nebula and present an allowed parameter space for its age and the radius of the putative nebula powering the observed PRS emission. …”
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357
THE STATE OF THE WARM AND COLD GAS IN THE EXTREME STARBURST AT THE CORE OF THE PHOENIX GALAXY CLUSTER (SPT-CLJ2344-4243)
Published 2015“…These new data reveal a complex emission-line nebula, extending for >30 kpc from the central galaxy, detected at [O II]λλ3726, 3729, [O III]λλ4959, 5007, Hβ, Hγ, Hδ, [Ne III]λ3869, and He II λ4686. …”
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358
Sea slugs (Gastropoda: Heterobranchia) from Rio Grande do Norte, Northeastern Brazil
Published 2022-12-01“…Marcus, 1967); Thuridilla malaquita Ortea & Buske, 2014; Berthella nebula Ghanimi, Schrödl, Goddard, Ballesteros, Gosliner & Valdés, 2020 and Berthella vialactea Ghanimi, Schrödl, Goddard, Ballesteros, Gosliner & Valdés, 2020. …”
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359
A Velocity Structure Analysis of Giant Molecular Cloud Associated with HII Region S152
Published 2005-06-01“…S152 is a small bright emission nebula located in the Perseus arm. Its optical diameter corresponds to 1.5 pc for an adopted distance 3.5 kpc. …”
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360
Herpetic Keratitis Following Corneal Crosslinking for Keratoconus: A Case Series
Published 2022-11-01“…All patients responded well to antiviral therapy, topical steroids, and epithelial nourishment medication, leaving corneal macula or nebula at the last follow-up visit.Conclusion: Close follow-up is essential and the most effective way to diagnose herpetic keratitis after corneal crosslinking due to the lack of subjective symptoms. …”
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