Works matching IS 00046264 AND DT 2022 AND VI 74 AND IP 3
Results: 16
Detection of highly correlated optical and X-ray variations in SS Cygni with Tomo-e Gozen and NICER.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. L17, doi. 10.1093/pasj/psac027
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- Article
Suzaku observations of Fe K-shell lines in the supernova remnant W 51 C and hard X-ray sources in the proximity.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 656, doi. 10.1093/pasj/psac026
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- Article
Three-dimensional geometry and dust/gas ratios in massive star-forming regions over the entire LMC as revealed by the IRSF/SIRIUS survey.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 639, doi. 10.1093/pasj/psac025
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Detection of gamma-rays around SNR HB9 and its implications for the diffusive shock-acceleration history.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 625, doi. 10.1093/pasj/psac024
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Passive spiral galaxies deeply captured by Subaru Hyper Suprime-Cam.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 612, doi. 10.1093/pasj/psac023
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NuSTAR discovery of the hard X-ray emission and a wide-band X-ray spectrum from the Pictor A western hotspot.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 602, doi. 10.1093/pasj/psac022
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symbiotic and bipolar nebula M 2-9: Morphological variability of the collimated ionized wind arising from the core.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 594, doi. 10.1093/pasj/psac020
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Thirty Millimeter Telescope.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 578, doi. 10.1093/pasj/psac019
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Detection of nitrogen and oxygen in a galaxy at the end of reionization.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. L9, doi. 10.1093/pasj/psac018
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- Article
Activity of the post-nova V1363 Cygni on long timescales.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 569, doi. 10.1093/pasj/psac017
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- Article
Is there a low-mass triple system orbiting around the massive semi-detached binary ZZ Cassiopeiae?
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 533, doi. 10.1093/pasj/psac016
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- Article
Ammonia mapping observations toward the Galactic massive star-forming region Sh 2-255 and Sh 2-257.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 545, doi. 10.1093/pasj/psac014
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Measurements of chromospheric Mg i emission lines of zero-age main-sequence stars.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 557, doi. 10.1093/pasj/psac013
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Physical properties of the molecular cloud, N4, in SS 433: Evidence for an interaction of molecular cloud with the jet from SS 433.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 493, doi. 10.1093/pasj/psac012
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X-ray hot spots in the eastern ear of the supernova remnant W 50 and the microquasar SS 433 system.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 510, doi. 10.1093/pasj/psac011
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Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 3, p. 521, doi. 10.1093/pasj/psac010
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- Article