To study some characteristics of the interstellar medium, observa- tional data of pulsars with large Faraday rotation values ( jRMj > 300 rad / m2) were used. It was suggested and justified that large jRMj values can be due to the contribution of the regions with increased electron concentration, projected on the pulsar. Most likely these are the HII regions, dark nebulae and molecular clouds. In these objects the magnetic field can be oriented in the direction of a large-scale field of the Galaxy, or simply is a deformed extension of the galactic field. It was shown that the Galactic distribution of rotation measures of pulsars with jRMj > 300 rad m2 corresponds to the circular model of the magnetic field of the Galaxy, with the counter-clockwise direction of the magnetic field in the galactocentric circle 5 kpc < R < 7 kpc.
oai:arar.sci.am:293883
ՀՀ ԳԱԱ Հիմնարար գիտական գրադարան
Aug 1, 2024
Dec 21, 2021
8
https://arar.sci.am/publication/321196
Mickaelian, A. M. Abrahamyan, H. V. Paronyan, G. M. Mikayelyan, G. A. Andreasyan, R. R. Sukiasyan A. G. Hambardzumyan, L. A. Mkrtchyan, V. K. Gasparyan, A. A.
Hovhannisyan, M. A. Andreasyan, R. R. Paronyan, G. M. Abrahamyan, H. V.
Mickaelian, A. M. Mikayelyan, G. A. Abrahamyan, H. V. Paronyan, G. M.
Andreasyan, R. R. Hakopian, S. A. Mahtessian, A. P. Abrahamyan, H. V. Paronyan, G. M. Sukiasyan, A. G.
Mickaelian, A. M. Abrahamyan, H. V. Paronyan, G. M. Mikayelyan, G. A.
Mikayelyan, G. A. Paronyan, G. M. Azatyan, N. M. Kostandyan, G. R. Samsonyan, A. L. Andreasyan, H. R. Abrahamyan, H. V. Andreasyan, D. H. Suqiasyan, A. G. Mickaelian, A. M.
Mickaelian, A. M. Abrahamyan, H. V. Paronyan, G. M. Mikayelyan, G. A. Andreasyan, R. R. Sukiasyan, A. G. Hambardzumyan, L. A. Mkrtchyan, V. K.
Mickaelian, A. M. Gigoyan, K. S. Gyulzadyan, M. V. Paronyan, G. M. Abrahamyan, H. V. Andreasyan, H. R. Azatyan, N. M. Kostandyan, G. R. Samsonyan, A. L. Mikayelyan, G. A. Farmanyan, S. V. Harutyunyan, V. L.