Zobrazeno 1 - 10
of 153
pro vyhledávání: '"Lamzin, S"'
Autor:
Dodin, A. V., Potanin, S. A., Burlak, M. A., Cheryasov, D. V., Ikonnikova, N. P., Lamzin, S. A., Safonov, B. S., Shatskii, N. I., Tatarnikov, A. M.
Publikováno v:
A&A, 684, L25, 2024
A strong global magnetic field of young low-mass stars and a high accretion rate are the necessary conditions for the formation of collimated outflows (jets) from these objects. But it is still unclear whether these conditions are also sufficient. We
Externí odkaz:
http://arxiv.org/abs/2404.06491
Publikováno v:
Physics-Uspekhi, 66(4), 327-359 (2023)
Jets from young stars are used as an example to review how laboratory modeling enables advancement in understanding the main physical processes responsible for the formation and stability of these amazing objects. The discussion focuses on the option
Externí odkaz:
http://arxiv.org/abs/2307.08491
Autor:
Belinski, A., Burlak, M., Dodin, A., Emelyanov, N., Ikonnikova, N., Lamzin, S., Safonov, B., Tatarnikov, A.
We present the results of our new observations of the young binary ZZ Tau with a circumbinary disc. The system was found to consist of two coeval (age $<2$ Myr) classical T Tauri stars with the total mass $0.86 \pm 0.09$ M$_\odot$, orbital period $46
Externí odkaz:
http://arxiv.org/abs/2206.14154
The secondary of the famous young binary RW Aur is much less studied than the primary. To compensate this shortcoming, we present here the results of UBVRIJHK photometric, VRI polarimetric and optical spectral observations of RW Aur B. The star demon
Externí odkaz:
http://arxiv.org/abs/2007.12559
Autor:
Dodin, A., Grankin, K., Lamzin, S., Nadjip, A., Safonov, B., Shakhovskoi, D., Shenavrin, V., Tatarnikov, A., Vozyakova, O.
Publikováno v:
MNRAS, Vol. 482, p. 5524 (2019)
Results of $UBVRIJHKLM$ photometry and $VRI$ polarimetry of a young star RW Aur A observed during unprecedented long and deep (up to $\Delta V \approx 5$ mag) dimming events in 2010-11 and 2014-18 are presented. The polarization degree $p$ of RW Aur
Externí odkaz:
http://arxiv.org/abs/1811.00449
Autor:
Berdnikov, L. N., Burlak, M. A., Vozyakova, O. V., Dodin, A. V., Lamzin, S. A., Tatarnikov, A. M.
Comparing the images of the jet of the young star RW Aur A, separated by a period of 21.3 years, we found that the outermost jet's knots have emerged $\approx 350$ yr ago. We argue that at that moment the jet itself has appeared and intensive accreti
Externí odkaz:
http://arxiv.org/abs/1708.08488
Autor:
Lamzin, S., Cheryasov, D., Chuntonov, G., Dodin, A., Grankin, K., Malanchev, K., Nadzhip, A., Safonov, B., Shakhovskoy, D., Shenavrin, V., Tatarnikov, A., Vozyakova, O.
Publikováno v:
ASP Conf. Ser. v.510, p.356 (2017)
Results of UBVRIJHKLM photometry, VRI polarimetry and optical spectroscopy of a young star RW Aur A obtained during 2010-11 and 2014-16 dimming events are presented. During the second dimming the star decreased its brightness to \Delta V > 4.5 mag, p
Externí odkaz:
http://arxiv.org/abs/1707.09671
Autor:
Nadjip, A. E., Tatarnikov, A. M., Toomey, D. W., Shatsky, N. I., Cherepashchuk, A. M., Lamzin, S. A., Belinski, A. A.
Publikováno v:
Astroph. Bull, 72, issue 3, p.349, 2017
ASTRONIRCAM is a cryogenic-cooled slit spectrograph for the spectral range 1-2.5 mkm installed at the Nasmyth focus of the 2.5-meter telescope of the Caucasian observatory of Sternberg Astronomical Institute of Lomonosov Moscow State University. The
Externí odkaz:
http://arxiv.org/abs/1706.08959
Akademický článek
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Autor:
Dodin, A. V., Emelyanov, N. V., Zharova, A. V., Lamzin, S. A., Malogolovets, E. V., Roe, J. M.
The results of our speckle interferometric observations of young binaries VY Tau and XZ Tau are presented. For the first time, we found a relative displacement of VY Tau components as well as a preliminary orbit for XZ Tau. It appeared that the orbit
Externí odkaz:
http://arxiv.org/abs/1509.04966