Maqola

Study asymmetry of stellar jets

S. MelnikovNational University of Uzbekistan, Tashkent, UzbekistanK. T. MirtadjievaAstronomical Institute of Uzbek Academy of Science, Tashkent, Uzbekistan

Bulletin of National University of Uzbekistan Mathematics and Natural Sciencesjournal2021en

ABI

Annotatsiya

This review article describes the diversity of astrophysical jets. The differences between relativistic and slower stellar jets are described briefly. The data on recent studies of stellar jets, which led to the discovery of the asymmetry of their emissions - a mismatch of their parameters in the opposite components. A review of the physical mechanisms that is proposed to explain the observed asymmetry is given.

Mavzular

Gamma-ray bursts and supernovae Astrophysics and Cosmic Phenomena Astro and Planetary Science

Identifikatorlar

DOI: 10.56017/2181-1318.1206

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