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Dive into the research topics where N. I. Shatsky is active.

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Featured researches published by N. I. Shatsky.


Monthly Notices of the Royal Astronomical Society | 2017

The curtain remains open: NGC 2617 continues in a high state

V.L. Oknyansky; C.M. Gaskell; N.A. Huseynov; V. Lipunov; N. I. Shatsky; Sergey S. Tsygankov; E. Gorbovskoy; K.M. Mikailov; A. M. Tatarnikov; D.A. Buckley; V.G. Metlov; A. E. Nadzhip; A. Kuznetsov; P.V. Balanutza; Burlak; G.A. Galazutdinov; B. P. Artamonov; I.R. Salmanov; Konstantin Malanchev; R.S. Oknyansky

Optical and near-infrared photometry, optical spectroscopy, and soft X-ray and UV monitoring of the changing look active galactic nucleus NGC 2617 show that it continues to have the appearance of a type-1 Seyfert galaxy. An optical light curve for 2010-2016 indicates that the change of type probably occurred between 2010 October and 2012 February and was not related to the brightening in 2013. In 2016 NGC 2617 brightened again to a level of activity close to that in 2013 April. We find variations in all passbands and in both the intensities and profiles of the broad Balmer lines. A new displaced emission peak has appeared in H


Astronomy Letters | 2016

Meteorological conditions at the Caucasus Observatory of the SAI MSU from the results of the 2007–2015 campaign

Victor G. Kornilov; M.V. Kornilov; N. I. Shatsky; O. V. Vozyakova; I. Gorbunov; B. S. Safonov; S. A. Potanin; D. V. Cheryasov; V. Senik

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Astronomy Reports | 2017

Analysis of the optics of the 2.5-m telescope of the Sternberg Astronomical Institute

S. A. Potanin; I. Gorbunov; A. V. Dodin; A. D. Savvin; B. S. Safonov; N. I. Shatsky

. X-ray variations are well correlated with UV-optical variability and possibly lead by


Odessa Astronomical Publications | 2016

THE CHANGING LOOK AGNS MONITORING PROJECT

V. L. Oknyanskij; N.A. Huseynov; V. Lipunov; A. M. Tatarnikov; N. I. Shatsky; Sergey S. Tsygankov; V.G. Metlov; I.R. Salmanov; C.M. Gaskell

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Monthly Notices of the Royal Astronomical Society | 2016

Night-sky brightness and extinction at Mt Shatdzhatmaz

Victor G. Kornilov; M.V. Kornilov; O. Voziakova; N. I. Shatsky; B. S. Safonov; I. Gorbunov; S. A. Potanin; D. V. Cheryasov; V. Senik

2-3 d. The


Monthly Notices of the Royal Astronomical Society | 2012

A study of the interacting binary system V455 Cygni

G. Djurašević; I. Vince; Igor I. Antokhin; N. I. Shatsky; A. Cséki; M. Zakirov; M. Eshankulova

K


Archive | 2017

Optical and J,K-photometry of black hole X-ray nova A0620-00 in passive and active stages of quiescence

Anatolii M. Cherepashchuk; Nataly A. Katysheva; T. S. Khruzina; S. Yu. Shugarov; A. M. Tatarnikov; M. A. Burlak; N. I. Shatsky

band lags the


Archive | 2017

The light curves of type II-P SN 2017eaw: first 200 days

D. Yu. Tsvetkov; S. Yu. Shugarov; Igor M. Volkov; N. N. Pavlyuk; O. V. Vozyakova; N. I. Shatsky; A. A. Nikiforova; I. S. Troitsky; Yu. V. Troitskaya; P. V. Baklanov

J


XXXIII Всероссийская конференция "Актуальные проблемы внегалактической астрономии"; Задачи научной программы обсерватории "Миллиметрон". Тезисы докладов | 2016

The curtain is still open: NGC 2617 remains in a high state

V.L. Oknyansky; B. P. Artamonov; N.A. Huseynov; V. Lipunov; E. Gorbovskoy; A. Kuznetsov; P.V. Balanutza; A. M. Tatarnikov; V.G. Metlov; N. I. Shatsky; A.E. Nadzhip; Burlak; K.M. Mikailov; C.M. Gaskell

band by about 21.5


The astronomer's telegram | 2016

The changing-type Seyfert NGC 2617 remains in a high state

V.L. Oknyansky; N.A. Huseynov; B. P. Artamonov; V. Lipunov; E. Gorbovskoy; A. Kuznetsov; P.V. Balanutza; A. M. Tatarnikov; V.G. Metlov; N. I. Shatsky; A.E. Nadzhip; Burlak; K.M. Mikailov; I.R. Salmanov; C.M. Gaskell

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V. Lipunov

Moscow State University

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V.G. Metlov

Moscow State University

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C.M. Gaskell

University of California

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N.A. Huseynov

National Academy of Sciences

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A. Kuznetsov

Moscow State University

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Burlak

Moscow State University

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