Search Results - "Atapin, K"
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Optical Counterparts of Ultraluminous X-Ray Sources NGC 4559 X-10 and NGC 4395 ULX-1
Published in The Astrophysical journal (20-02-2018)“…We study the optical counterparts of ultraluminous X-ray sources (ULXs) NGC 4559 X-10 and NGC 4395 ULX-1. Their absolute magnitudes, after taking reddening…”
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2
Ultraluminous X-Ray Sources
Published in Astrophysical bulletin (2021)“…Ultraluminous X-ray sources (ULXs) were identified as a separate class of objects in 2000 based on data from the Chandra X-Ray Observatory. These are unique…”
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I -band photometry of the quiescent black hole X-ray nova GROJ0422 + 32 = V518 Per: modelling of the orbital light curve and estimation of the black hole mass
Published in Monthly notices of the Royal Astronomical Society (25-06-2024)“…ABSTRACT We present new photometric observations of the X-ray nova GRO J0422 + 32 (V518 Per) carried out in the I$_c$ band over 14 nights in 2020–2023. We had…”
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4
Search for LBVs in the Local Volume galaxies: study of two stars in NGC 1156
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…ABSTRACT We continue the search for luminous blue variables (LBVs) in Local Volume galaxies in order to study their fundamental parameters. In this paper, we…”
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The Nature of the Emission Spectrum of NGC 7793 P13: Testing the Supercritical Accretion Disk Wind Model
Published in Astrophysical bulletin (01-09-2023)“…The optical spectra of ultraluminous X-ray sources (ULXs) show signs of powerful outflows of matter. These outflows are responsible for the formation of a…”
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6
New luminous blue variable candidates in the NGC 247 galaxy
Published in Monthly notices of the Royal Astronomical Society (01-10-2020)“…ABSTRACT We search for luminous blue variable (LBV) stars in galaxies outside the Local Group. Here we present a study of two bright Hα sources in the NGC 247…”
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Post-AGB candidate IRAS 02143+5852: Cepheid-like variability, three-layer circumstellar dust envelope and spectral features
Published in Monthly notices of the Royal Astronomical Society (13-04-2024)“…ABSTRACT We present the results of multicolour UBVRCICJHK photometry, spectroscopic analysis and spectral energy distribution (SED) modelling for the post-AGB…”
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8
Investigation of the Ultraluminous X-ray Source VII Zw 403 ULX in the X-ray and Optical Ranges
Published in Astronomy letters (01-12-2023)“…We present the results of our analysis of the series of X-ray observations, photometric and spectroscopic monitoring for the ultraluminous X-ray source VII Zw…”
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9
Optical counterparts of ULXs in two dwarf galaxies: NGC 4861 and NGC 4449
Published in Monthly notices of the Royal Astronomical Society (01-07-2021)“…ABSTRACT We present the results of a search for optical candidates of ultraluminous X-ray sources (ULXs) in two dwarf galaxies, NGC 4861 and NGC 4449, using…”
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10
Search for LBVs in the Local Volume galaxies: study of four stars in NGC 4449
Published in Monthly notices of the Royal Astronomical Society (01-11-2021)“…ABSTRACT We continue to search for LBV stars in galaxies outside the Local Group. In this work, we have investigated four luminous stars in NGC 4449. Multiple…”
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11
Nature of the Emission Spectrum of NGC 7793 P13: Modeling the Atmosphere of the Donor Star
Published in Astrophysical bulletin (2024)“…We continue to study the ultra-luminous X-ray source NGC 7793 P13 in the optical range. In this work, we are testing the model of a spherically symmetric wind…”
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12
X-ray variability of SS 433: Evidence for supercritical accretion
Published in Astronomy letters (01-08-2016)“…We study the X-ray variability of SS 433 based on data from the ASCA observatory and the MAXI and RXTE/ASM monitoring missions. Based on the ASCA data, we have…”
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13
New luminous blue variable candidates in NGC 4736
Published in Monthly notices of the Royal Astronomical Society. Letters (21-03-2019)“…ABSTRACT We have found three new luminous blue variable (LBV) candidates in the star-forming galaxy NGC 4736. They show typical well-known LBV spectra, broad…”
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14
Modeling of Extended Atmospheres with Temperatures below 40000 K
Published in Astrophysical bulletin (01-04-2020)“…We calculate models of extended stellar atmospheres with a temperature in the range of 12 000–40 000 K and a mass loss rate of – . A large number of objects…”
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15
Ultra-luminous X-ray sources as supercritical accretion disks: Spectral energy distributions
Published in Astrophysical bulletin (01-04-2013)“…We describe a model of spectral energy distribution in supercritical accretion disks (SCAD) based on the conception by Shakura and Sunyaev. We apply this model…”
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The Post-AGB Star IRAS 07253–2001: Pulsations, Long-Term Brightness Variability and Spectral Peculiarities
Published in Astrophysical bulletin (01-09-2023)“…The observations and comprehensive study of intermediate initial mass stars at the late stages of evolution, and after the asymptotic giant branch (AGB) in…”
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17
Search for Tidal Disruption Events Based on the SRG/eROSITA Survey with Subsequent Optical Spectroscopy
Published in Astronomy letters (01-12-2022)“…The four completed six-month sky surveys with the eROSITA telescope onboard the SRG orbital observatory allow tidal disruption events (TDEs) in galactic nuclei…”
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Simultaneous X-ray/UV Observations of Ultraluminous X-ray Source Holmberg II X-1 with Indian Space Mission Astrosat
Published in Astrophysical bulletin (01-09-2022)“…We present the results of eight epochs of simultaneous UV and X-ray observations of the highly variable ultraluminous X-ray source (ULX) Holmberg II X-1 with…”
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Optical Spectroscopy of SRG/eROSITA Objects with 2.5-m Telescope at the Caucasus Mountain Observatory of the SAI MSU
Published in Astronomy letters (01-07-2020)“…Based on observations with the new transient double-beam spectrograph (TDS) at the 2.5-m telescope of the Caucasus Mountain Observatory of SAI MSU, we have…”
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Optical Spectroscopy of Quasars Discovered by SRG/eROSITA with a 2.5-m Telescope at the Caucasus Mountain Observatory of SAI MSU
Published in Astronomy letters (01-10-2021)“…Based on observations with the transient double-beam spectrograph (TDS) at the 2.5-m telescope of the Caucasus Mountain Observatory of SAI MSU, we have…”
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