Broadband X-ray spectrum of the intermediate polar V2400 OphWe present the results of our analysis of the observations of the intermediate polar
V2400 Oph
Broadband X-ray spectrum of the intermediate polar V2400 OphWe present the results of our analysis of the observations of the intermediate polar
V2400 Oph
Variability of X-ray pulsars in a hard energy band observed with INTEGRAL variable X-ray flux (18-60 ke
V) from the pulsar EXO1722-363, which could be connected with the orbital
Variability of X-ray pulsars in a hard energy band observed with INTEGRAL variable X-ray flux (18-60 ke
V) from the pulsar EXO1722-363, which could be connected with the orbital
Coordinated integral and optical observations of SS433Cherepashchuk A.,
Sunyaev R.,
Fabrikat S.,
Molkov S.,
Barsukova E.,
Antokhina E.,
Irsmambetova T.,
Panchenko I.,
Postnov K.,
Seifina E.,
Shakura N.,
Timokhin A.,
Bikmaev I.,
Sakhibullin N.,
Gnedin Y.,
Arkharov A.,
Larionov V. radial velocity semiamplitude Kv = 132 km/
s. A strong heating effect in the optical star atmosphere
Observations of Her X-1 in low states during SRG/eROSITA all-sky survey of the optical star. The latter region effectively scatters photons with energies above 5-6 ke
V.
Coordinated integral and optical observations of SS433Cherepashchuk A.,
Sunyaev R.,
Fabrikat S.,
Molkov S.,
Barsukova E.,
Antokhina E.,
Irsmambetova T.,
Panchenko I.,
Postnov K.,
Seifina E.,
Shakura N.,
Timokhin A.,
Bikmaev I.,
Sakhibullin N.,
Gnedin Y.,
Arkharov A.,
Larionov V. radial velocity semiamplitude Kv = 132 km/
s. A strong heating effect in the optical star atmosphere
INTEGRAL observations of SS433: Results of a coordinated campaignCherepashchuk A.,
Sunyaev R.,
Fabrika S.,
Postnov K.,
Molkov S.,
Barsukova E.,
Antokhina E.,
Irsmambetova T.,
Panchenko I.,
Seifina E.,
Shakura N.,
Timokhin A.,
Bikmaev I.,
Sakhibullin N.,
Aslan Z.,
Khamitov I.,
Pramsky A.,
Sholukhova O.,
Gnedin Y.,
Arkharov A.,
Larionov V. with a maximum to minimum uneclipsed hard X-ray flux ratio of ∼4 is discovered. The 18-60 ke
V X
INTEGRAL observations of SS433: Results of a coordinated campaignCherepashchuk A.,
Sunyaev R.,
Fabrika S.,
Postnov K.,
Molkov S.,
Barsukova E.,
Antokhina E.,
Irsmambetova T.,
Panchenko I.,
Seifina E.,
Shakura N.,
Timokhin A.,
Bikmaev I.,
Sakhibullin N.,
Aslan Z.,
Khamitov I.,
Pramsky A.,
Sholukhova O.,
Gnedin Y.,
Arkharov A.,
Larionov V. with a maximum to minimum uneclipsed hard X-ray flux ratio of ∼4 is discovered. The 18-60 ke
V X