Zobrazeno 1 - 10
of 64
pro vyhledávání: '"A. V. Dodin"'
Autor:
G. A. Khorunzhev, S. Yu. Sazonov, P. S. Medvedev, M. R. Gilfanov, K. E. Atapin, A. A. Belinski, O. V. Vozyakova, A. V. Dodin, B. S. Safonov, A. M. Tatarnikov, I. F. Bikmaev, R. A. Burenin, S. N. Dodonov, M. V. Eselevich, I. A. Zaznobin, R. A. Krivonos, R. I. Uklein, K. A. Postnov, R. A. Sunyaev
Publikováno v:
Astronomy Letters. 48:767-789
Publikováno v:
Plasma Physics Reports. 48:606-617
Autor:
A. M. Cherepashchuk, A. V. Dodin, K. A. Postnov, A. A. Belinski, M. A. Burlak, N. P. Ikonnikova, T. R. Irsmambetova, S. A. Trushkin
Publikováno v:
Astronomy Reports. 66:451-465
Autor:
B. S. Safonov, A. V. Dodin
Publikováno v:
Astronomy Letters. 48:293-302
Publikováno v:
Astronomy Letters. 48:38-46
Autor:
A. V. Dodin, N. I. Shatsky, A. A. Belinski, K. E. Atapin, M. A. Burlak, S. G. Zheltoukhov, A. M. Tatarnikov, K. A. Postnov, A. M. Cherepashchuk, M. I. Belvedersky, V. D. Borisov, R. A. Burenin, M. R. Gilfanov, R. A. Krivonos, P. S. Medvedev, A. V. Meshcheryakov, S. Yu. Sazonov, R. A. Sunyaev, G. A. Khorunzhev
Publikováno v:
Astronomy Letters. 47:661-673
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 507:L19-L23
The examination of long-term (1979-2020) photometric observations of SS433 enabled us to discover a non-zero orbital eccentricity of $e=0.05\pm 0.01.$ We have also found evidence for a secular increase in the orbital period at a rate of $\dot P_\math
Autor:
N. P. Ikonnikova, V. I. Shenavrin, V. F. Esipov, A. M. Tatarnikov, G. V. Komissarova, A. V. Dodin, A. A. Belinskii, I.A. Shaposhnikov, S. G. Zheltoukhov, M. A. Burlak
Publikováno v:
Astronomy Letters. 47:485-504
We present the results of a UBVRcIc and JHKLM photometric monitoring campaign conducted in 2016–2020, low-resolution spectroscopy, and an analysis of the ASAS-3 and ASAS-SN photometric data for the semiregular variable and post-AGB candidate AU Vul
Publikováno v:
Astronomy Reports. 65:477-487
The use of Z-pinch facilities makes it possible to carry out well-controlled and diagnosable laboratory experiments to study laboratory jets with scaling parameters close to those of the jets from young stars. This makes it possible to observe proces
Publikováno v:
Astronomy Letters. 46:601-611
H 3-75 is a medium-excitation planetary nebula with a binary central star consisting of a hot subdwarf with $$T_{\textrm{hot}}\sim 10^{5}$$ K and a cool giant. We present the results of our photometric and spectroscopic observations obtained in 2020