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X-ray applications and recent advances @ XLab Frascati
Dabagov, S. B., Hampai, D., Guglielmotti, V., Cappuccio, G., Gladkikh, Yu.
XLab Frascati is a facility open to external users for different X-ray analyses, ranging from
The accretion environment of supergiant fast X-ray transients probed with XMM-Newton
Bozzo E., Bernardini F., Ferrigno C., Falanga M., Romano P., Oskinova L.
correlation between the dynamic ranges in the X-ray fluxes and absorption column densities in supergiant fast
Vertical structure of the outer accretion disk in persistent low-mass X-ray binaries
Mescheryakov A., Shakura N., Suleimanov V.
equation by the Sobolev method. This approximation has a ≲10% accuracy in the range of X-ray photon
Model atmospheres of x-ray bursting neutron stars
Suleimanov V., Poutanen J., Revnivtsev M., Werner K.
We present an extended set of model atmospheres and emergent spectra of X-ray bursting neutron
Vertical structure of the outer accretion disk in persistent low-mass X-ray binaries
Mescheryakov A., Shakura N., Suleimanov V.
equation by the Sobolev method. This approximation has a ≲10% accuracy in the range of X-ray photon
The impact of neutron star spin on X-ray spectra
an observable imprint on the spectral properties of X-ray binaries. To evaluate this, we consider a sample
Ultraluminous X-Ray Sources
Fabrika S.N., Atapin K.E., Vinokurov A.S., Sholukhova O.N.
Ultraluminous X-ray sources (ULXs) were identified as a separate class of objects in 2000 based
Basic parameters of the helium-accreting X-ray bursting neutron star in 4U 1820-30
Suleimanov V., Kajava J., Molkov S., Nättilä J., Lutovinov A., Werner K., Poutanen J.
. The ultracompact low-mass X-ray binary 4U 1820-30 situated in the globular cluster NGC 6624 has an orbital period
Model atmospheres of x-ray bursting neutron stars
Suleimanov V., Poutanen J., Revnivtsev M., Werner K.
We present an extended set of model atmospheres and emergent spectra of X-ray bursting neutron
The Use of Streak Photography, X-Ray Radiography, and Radiometric and Spectrometric Measurements to Study Plasma Bunches Generated under Gyroresonant Interactions
Andreev V.V., Novitskii A.A., Chuprov D.V.
spectral ranges using streak photography and X-ray imaging techniques. The original method of accounting

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