Found: 11
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X-ray iron absorption line in Swift J1858.6−0814.
- Published in:
- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 98, doi. 10.1093/pasj/psad082
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- Article
Survivability of amorphous ice in comets depends on the latent heat of crystallization of impure water ice.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 130, doi. 10.1093/pasj/psad086
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- Article
Survey of public attitudes toward astronomy in Japan.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 108, doi. 10.1093/pasj/psad084
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- Article
Absolute properties of the oscillating eclipsing Algol XZ Ursae Majoris.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 118, doi. 10.1093/pasj/psad085
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- Article
The variability of the broad line profiles of SDSS J1430+2303.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 103, doi. 10.1093/pasj/psad083
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- Article
The history of the Milky Way: The evolution of star formation, cosmic rays, metallicity, and stellar dynamics over cosmic time.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 81, doi. 10.1093/pasj/psad081
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- Article
KAgoshima Galactic Object survey with Nobeyama 45 m telescope by Mapping in Ammonia lines (KAGONMA): Discovery of parsec-scale CO depletion in the Canis Major star-forming region.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 65, doi. 10.1093/pasj/psad080
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- Article
Tentative detection of cyanoformamide NCCONH2 in space.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 54, doi. 10.1093/pasj/psad079
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- Article
Sulfur isotopes toward the extended envelope of Sagittarius B2 in the Galactic Center.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 46, doi. 10.1093/pasj/psad078
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- Article
HINOTORI I: The nature of rejuvenation galaxies.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 1, doi. 10.1093/pasj/psad076
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- Article
Magnetic activity variability of nearby bright Sun-like stars by 4 yr intensive Hα line monitoring.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 1, p. 27, doi. 10.1093/pasj/psad077
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- Publication type:
- Article