activity
20092026
most citedMulti-Wavelength Monitoring and Reverberation Mapping of a Changing Look Event in the Seyfert Galaxy NGC 3516

34 citations · 218 across the 44 of their papers we have counts for

collaborators

45 papers

astro-ph.SR2026

First double red giant Algol system with active mass transfer

Mikhail Kovalev, Hailiang Chen, Sufen Guo +7

Double red giant stars are very important for studies of the stability of mass transfer, common-envelope evolution, and the formation of double white dwarfs with short orbital peri…

astro-ph.SR2026

Photometric and spectral variability of the candidate post-AGB star IRAS 07506-0345

N. P. Ikonnikova, M. A. Burlak, A. V. Dodin

We report photometric and spectroscopic observations of the poorly studied post-AGB candidate IRAS 07506-0345, obtained with the telescopes of the Caucasian Mountain Observatory of…

astro-ph.SR2026

The curved jet in the young star FN Tau

M. A. Burlak, A. V. Dodin, A. V. Zharova +5

In the vicinity of the young star FN Tau, we have detected a microjet and four Herbig-Haro objects, whose positions and kinematics indicate the presence of a bipolar collimated out…

astro-ph.HE2026

Anomaly detection in Fink. I. Discovery, follow-up, and classification of unusual sources

M. V. Pruzhinskaya, M. V. Kornilov, A. V. Dodin +19

Modern wide-field time-domain surveys produce alert streams whose scientific potential is often concentrated in rare and unusual events. Efficient discovery therefore requires auto…

astro-ph.SR2026

Photometric and Spectral Evolution of the Symbiotic Nova HM Sagittae since 2003

N. P. Ikonnikova, V. I. Shenavrin, G. V. Komissarova +2

We present photometric and spectral monitoring of the symbiotic system HM Sge, which consists of a Mira variable with a dust shell and a hot white dwarf ionizing the surrounding ga…

astro-ph.SR2026

The eruptive young star IRAS 21204+4913

M. A. Burlak, A. V. Dodin, A. V. Zharova +7

The results of photometric, polarimetric, and spectroscopic observations are presented for the young star IRAS 21204+4913, whose visible brightness has increased by $\approx 5^{\rm…

astro-ph.SR2025★ 2 cited

Photometric Analysis of TCP J201712881156589 -- WZ Sge Type Dwarf Nova with Delayed Ordinary Superhumps Emergence

Alexander Tarasenkov, Sergey Shugarov, Natalia Ikonnikova +3

We present the results of photometric analysis of WZ Sge type dwarf nova TCP J201712881156589. This object exhibited an outburst with a large amplitude of magnitudes and…

astro-ph.SR2025

On the influence of component orbital motion on the photometric variability of DF Tau

M. A. Burlak, K. N. Grankin, A. V. Dodin +6

Based on the analysis of the long-term light curve of the young binary DF Tau spanning approximately 125 years, we infer that its brightness variations are associated with changes…

astro-ph.SR2025

IRAS 22272+5435 (V354 Lac): Multicolor Photometry of a Variable Carbon-rich post-AGB Star and a Dust Formation Episode

N. P. Ikonnikova, V. I. Shenavrin, G. V. Komissarova +1

We present new UBV photometric observations (2009-2024) of the carbon-rich post-AGB star IRAS 22272+5435 (V354 Lac), combined with our data spanning over 30 years (1991-2024). The…

astro-ph.GA2025

Broad line region echo from highly accreting intermediate-mass black hole candidate SDSS J144850.08+160803.1. The first probe of intra-night variability and reverberation mapping

Mariia Demianenko, Anton Afanasiev, Evgenii Rubtsov +8

Elusive intermediate-mass black holes (IMBHs) can be used as ``time-squeezing'' machines, enabling studies of AGN geometry via reverberation mapping on much shorter timescales than…

astro-ph.SR2025

On the causes of brightness variability of the young star BP Tau

M. A. Burlak, K. N. Grankin, A. V. Dodin +6

We have constructed and analysed the secular light curve of BP Tau, a classical T Tauri-type star. Wave-like variations in the average brightness were detected, with an amplitude o…

astro-ph.HE2025★ 1 cited

Optical and X-ray timing analysis of the 2018-2020 outburst and rebrightening of the black-hole transient MAXI J1820+070

M. Fiori, L. Zampieri, A. Burtovoi +15

We report the results of a comprehensive analysis of the multiwavelength (in optical and X-rays) and multitimescale (from months to tenths of a second) variability of the 2018-2020…

astro-ph.IM2025

The BVRcIc sky brightness of the Caucasian Mountain Observatory of MSU

I. A. Komarova, A. M. Tatarnikov, A. V. Sharonova +4

In this paper we analyse the measurements of the brightness of the night sky above the CMO SAI MSU in the visible and near-infrared range made in 2019-2014. In 2023-2024 the median…

astro-ph.SR2024

MASTER OT J030227.28+191754.5: an unprecedentedly energetic dwarf nova outburst

Yusuke Tampo, Taichi Kato, Keisuke Isogai +60

We present a detailed study of the MASTER OT J030227.28+191754.5 outburst in 2021-2022, reaching an amplitude of 10.2 mag and a duration of 60 d. The detections of (1) the double-p…

astro-ph.SR2024

High-resolution spectroscopy of the variable hot post-AGB star LS 4331 (IRAS 17381-1616)

N. P. Ikonnikova, M. Parthasarathy, I. A. Shaposhnikov +2

An analysis of high-resolution () optical spectrum of hot (B1Ibe) post-AGB star LS 4331 (IRAS 17381-1616) is presented. The detailed identification of the observed ab…

astro-ph.SR2024★ 1 cited

Discovery of a hot post-AGB star in Galactic globular cluster E3

R. Kumar, A. Moharana, S. Piridi +8

We report a new hot post-asymptotic giant branch (PAGB) star in the Galactic globular cluster (GC) E3, which is one of the first of the identified PAGB stars in a GC to show a bina…

astro-ph.SR2024★ 2 cited

The jet of BP Tau

A. V. Dodin, S. A. Potanin, M. A. Burlak +6

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. Bu…

astro-ph.SR2024

Post-AGB candidate IRAS 02143+5852: Cepheid-like variability, three-layer circumstellar dust envelope and spectral features

N. P. Ikonnikova, M. A. Burlak, A. V. Dodin +8

We present the results of multicolour photometry, spectroscopic analysis and spectral energy distribution (SED) modelling for the post-AGB candidat…

astro-ph.SR2024★ 1 cited

ZZ Tau IRS: a low mass UX Ori type star with strong wind

M. A. Burlak, A. V. Dodin, A. V. Zharova +7

The results of photometric, polarimetric and spectroscopic observations of the young star ZZ Tau IRS in the visible and near-infrared bands are presented. Against the continuum of…

astro-ph.SR2023

TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections?

Kirill V. Sokolovsky, Elias Aydi, Konstantin Malanchev +70

Lightcurves of many classical novae deviate from the canonical "fast rise - smooth decline" pattern and display complex variability behavior. We present the first TESS-space-photom…

astro-ph.HE2023

Long-term multiwavelength monitoring and reverberation mapping of NGC 2617 during a changing-look event

V. L. Oknyansky, M. S. Brotherton, S. S. Tsygankov +32

We present the results of photometric and spectroscopic monitoring campaigns of the changing look AGN NGC~2617 carried out from 2016 until 2022 and covering the wavelength range fr…

astro-ph.SR2023

The Post-AGB Star IRAS 07253-2001: Pulsations, Long-Term Brightness Variability and Spectral Peculiarities

N. P. Ikonnikova, M. A. Burlak, A. V. Dodin +5

The observations and comprehensive study of intermediate initial mass stars at the late stages of evolution, and after the asymptotic giant branch (AGB) in particular, are of cruci…

astro-ph.SR2022★ 8 cited

Orbital parameters and activity of ZZ Tau -- a low mass young binary with circumbinary disc

A. Belinski, M. Burlak, A. Dodin +5

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 Myr) classical T Tauri s…

astro-ph.SR2022★ 1 cited

FG Sge: new multicolor photometry and short-term dust shell clearing in 2019

V. P. Arkhipova, N. P. Ikonnikova, V. I. Shenavrin +6

We present the results of a new stage of the long-term photometric study of FG Sge which is a quickly evolving central star of the planetary nebula Hen 1-5. Our new observations ca…