Observation of a Helioseismically Active Solar Flare with a Low Hard X-ray Flux up to 50 keV.
- Published in:
- Astronomy Letters, 2024, v. 50, n. 3, p. 203, doi. 10.1134/S1063773724700026
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- Publication type:
- Article
Works matching IS 10637737 AND DT 2024 AND VI 50 AND IP 3
Results: 5
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2
Increase in the Brightness of the Cosmic Radio Background toward Galaxy Clusters.
- Published in:
- Astronomy Letters, 2024, v. 50, n. 3, p. 159, doi. 10.1134/S1063773724700063
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- Publication type:
- Article
3
Erratum to: The Method of Periodic Principal Components for the Dynamic Spectrum of Radio Pulsars and Faraday Rotation of Nine Pulse Components of PSR B0329+54.
- Published in:
- 2024
- By:
- Publication type:
- Correction Notice
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Clumpy Accretion As a Possible Cause of Prolonged Eclipses in UX Ori Stars.
- Published in:
- Astronomy Letters, 2024, v. 50, n. 3, p. 194, doi. 10.1134/S1063773724700075
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- Publication type:
- Article
5
Annihilation of Positrons from AGN Jets As a Possible Source of Cosmic Gamma-Ray Background at Energies below 511 keV.
- Published in:
- Astronomy Letters, 2024, v. 50, n. 3, p. 186, doi. 10.1134/S1063773724700087
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- Publication type:
- Article