collaborators

6 papers

astro-ph20079 cited

High-Mass X-ray Binaries and the Spiral Structure of the Host Galaxy

P. Shtykovskiy, M. Gilfanov

We investigate the manifestation of the spiral structure in the distribution of high-mass X-ray binaries (HMXBs) over the host galaxy. We construct the simple kinematic model. It s…

astro-ph200730 cited

High Mass X-ray Binaries and Recent Star Formation History of the Small Magellanic Cloud

P. Shtykovskiy, M. Gilfanov

We study the relation between high-mass X-ray binary (HMXB) population and recent star formation history (SFH) for the Small Magellanic Cloud (SMC). Using archival optical SMC obse…

astro-ph2004

Constraints on the luminosity of the stellar remnant in SNR1987A

P. Shtykovskiy, A. Lutovinov, M. Gilfanov +1

We obtain photometric constraints on the luminosity of the stellar remnant in SNR1987A using XMM-Newton and INTEGRAL data. The upper limit in the 2--10 keV band based on the XMM-Ne…

astro-ph2004

High mass X-ray binaries in the LMC: dependence on the stellar population age and the "propeller" effect

P. Shtykovskiy, M. Gilfanov

We study population of compact X-ray sources in the Large Magellanic Cloud using the archival data of XMM-Newton observatory. The total area of the survey is approximately 3.8 squa…

astro-ph1999

The nature of SN 1997D: low-mass progenitor and weak explosion

Nikolai N. Chugai, Victor P. Utrobin

We analyzed the spectra and light curve of the peculiar type II-P supernova 1997D to recover ejecta parameters. The optimal hydrodynamical model of SN 1997D, which meets observatio…

astro-ph1998

76 mas speckle-masking interferometry of IRC+10216 with the SAO 6m telescope: Evidence for a clumpy shell structure

G. Weigelt, Y. Balega, T. Bloecker +3

We present the first K'-band image of the carbon star IRC+10216 with 76 mas resolution. The diffraction-limited image was reconstructed from 6m telescope speckle data using the spe…