Works matching IS 00046264 AND DT 2024 AND VI 76 AND IP 4
Results: 21
Dynamical properties of mildly relativistic ejecta produced by the mass-loading of gamma-ray burst jets in dense ambient media.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 863, doi. 10.1093/pasj/psae055
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First star formation in extremely early epochs.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 850, doi. 10.1093/pasj/psae054
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Searching for the signature of fast radio burst by Swift/XRT X-ray afterglow light curve.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 841, doi. 10.1093/pasj/psae053
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- Article
Impact of turbulent magnetic fields on disk formation and fragmentation in first star formation.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 823, doi. 10.1093/pasj/psae051
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- Article
Measurement of temperature relaxation in the postshock plasma of the northwestern limb of SN 1006.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 800, doi. 10.1093/pasj/psae049
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Cosmic very small dust grains as a natural laboratory of mesoscopic physics: Modeling thermal and optical properties of graphite grains.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 810, doi. 10.1093/pasj/psae050
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Dark supernova remnant buried in the Galactic Center "Brick" G0.253+0.016 revealed by an expanding CO-line bubble.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 773, doi. 10.1093/pasj/psae047
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Broad-band non-thermal emission of odd radio circles induced by explosive galactic outflow remnants and their evolution.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 765, doi. 10.1093/pasj/psae046
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Evolution of grain size distribution in the circumgalactic medium.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 753, doi. 10.1093/pasj/psae045
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- Article
Final results of the search for new Milky Way satellites in the Hyper Suprime-Cam Subaru Strategic Program survey: Discovery of two more candidates.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 733, doi. 10.1093/pasj/psae044
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A deep analysis for New Horizons' KBO search images.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 720, doi. 10.1093/pasj/psae043
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- Article
A self-consistent model for dust settling and the vertical shear instability in protoplanetary disks.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 708, doi. 10.1093/pasj/psae042
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- Article
On the X-ray efficiency of the white dwarf pulsar candidate ZTF J190132.9+145808.7.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 702, doi. 10.1093/pasj/psae041
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Discovery of free precession in the magnetar SGR 1806−20 with the ASCA Gas Imaging Spectrometer.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 688, doi. 10.1093/pasj/psae040
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Co-evolution of dust grains and protoplanetary disks. II. Structure and evolution of protoplanetary disks: An analytical approach.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 674, doi. 10.1093/pasj/psae039
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Physics of nova outbursts: Theoretical models of classical nova outbursts with optically thick winds on 1.2 M⊙ and 1.3 M⊙ white dwarfs.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 666, doi. 10.1093/pasj/psae038
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Efficient identification of broad absorption line quasars using dimensionality reduction and machine learning.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 653, doi. 10.1093/pasj/psae037
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Dynamics near the inner dead-zone edges in a proprotoplanetary disk.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 616, doi. 10.1093/pasj/psae036
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High-mass star formation in the Large Magellanic Cloud triggered by colliding H i flows.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 589, doi. 10.1093/pasj/psae035
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The CO-to-H2 conversion factor in the Central Molecular Zone of the Milky Way using CO isotopologues.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 579, doi. 10.1093/pasj/psae033
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An ultra wide-band, high-sensitivity Q-band receiver for single-dish telescopes, eQ: Rest-frequency determination of CCS (JN = 43–32) and SO (JN = 10–01) and high-redshift CO (J = 1–0) detection.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 563, doi. 10.1093/pasj/psae029
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