Sergey Tsygankov

Near-periodical spin period evolution in the binary system LMC X-4 (2017)

Monthly Notices of the Royal Astronomical Society

Molkov S, Lutovinov A, Falanga M, Tsygankov S, Bozzo E

(Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1))

Determination of the distance to SWIFT J0243.6+6124 (2017)

I. Bikmaev, V. Shimansky, E. Irtuganov, M. Glushkov, N. Sakhibullin, I. Khamitov, R. Burenin, A. Lutovinov, I. Zaznobin, M. Pavlinsky, R. Sunyaev, S. Dodonov, V. Afanasiev, S. Kotov, V. Doroshenko, S. Tsygankov

(Artikkeli ammatillisessa kokoomateoksessa (D2))

NuSTAR observations of the supergiant X-ray pulsar IGR J18027-2016: accretion from the stellar wind and possible cyclotron absorption line (2017)

Monthly Notices of the Royal Astronomical Society

Lutovinov AA, Tsygankov SS, Postnov KA, Krivonos RA, Molkov SV, Tomsick JA

(Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1))

Correlated X-ray and Optical Variability in Intermediate Polars During their Outbursts (2017)

European Workshop on White Dwarfs

Neustroev VV, Tsygankov S, Suleimanov V, Sjoberg G

(Vertaisarvioitu artikkeli konferenssijulkaisussa (A4))

Radius of the Neutron Star Magnetosphere during Disk Accretion (2017)

Astronomy Letters / Pis'ma v Astronomicheskii Zhurnal

Filippova EV, Mereminskiy IA, Lutovinov AA, Molkov SV, Tsygankov SS

(Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1))

Luminosity dependence of the cyclotron line and evidence for the accretion regime transition in V 0332+53 (2017)

Monthly Notices of the Royal Astronomical Society

Doroshenko V, Tsygankov SS, Mushtukov AA, Lutovinov AA, Santangelo A, Suleimanov VF, Poutanen J

(Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1))

High-precision optical polarimetry of the accreting black hole V404 Cyg during the 2015 June outburst (2017)

Monthly Notices of the Royal Astronomical Society

Ilia A. Kosenkov, Andrei V. Berdyugin, Vilppu Piirola, Sergey S. Tsygankov, Enric Pallé, Paulo A. Miles-Páez, Juri Poutanen

(Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1))

Expanding hot flow in the black hole binary SWIFT J1753.5-0127: evidence from optical timing (2017)

Monthly Notices of the Royal Astronomical Society

Veledina A, Gandhi P, Hynes R, Kajava JJE, Tsygankov SS, Revnivtsev MG, Durant M, Poutanen J

(Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1))

New hard X-ray sources discovered in the ongoing INTEGRAL Galactic plane survey after 14 yr of observations (2017)

Monthly Notices of the Royal Astronomical Society

Roman A. Krivonos, Sergey S. Tsygankov, Ilya A. Mereminskiy, Alexander A. Lutovinov, Sergey Yu. Sazonov, Rashid A. Sunyaev

(Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1))

SMC X-3: the closest ultraluminous X-ray source powered by a neutron star with non-dipole magnetic field (2017)

Astronomy and Astrophysics

Tsygankov SS, Doroshenko V, Lutovinov AA, Mushtukov AA, Poutanen J

(Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1))

Ota yhteyttä

Julkaisut

Järjestä:

Near-periodical spin period evolution in the binary system LMC X-4 (2017)

Determination of the distance to SWIFT J0243.6+6124 (2017)

NuSTAR observations of the supergiant X-ray pulsar IGR J18027-2016: accretion from the stellar wind and possible cyclotron absorption line (2017)

Correlated X-ray and Optical Variability in Intermediate Polars During their Outbursts (2017)

Radius of the Neutron Star Magnetosphere during Disk Accretion (2017)

Luminosity dependence of the cyclotron line and evidence for the accretion regime transition in V 0332+53 (2017)

High-precision optical polarimetry of the accreting black hole V404 Cyg during the 2015 June outburst (2017)

Expanding hot flow in the black hole binary SWIFT J1753.5-0127: evidence from optical timing (2017)

New hard X-ray sources discovered in the ongoing INTEGRAL Galactic plane survey after 14 yr of observations (2017)

SMC X-3: the closest ultraluminous X-ray source powered by a neutron star with non-dipole magnetic field (2017)