Vertical structure of the outer accretion disk in persistent low-mass X-ray binaries accretion disk in low-mass X-ray binaries by performing
a self-consistent calculation of the vertical
Additional spectroscopic redshift measurements for galaxy clusters from the first Planck catalogueVorobyev V.,
Burenin R.,
Bikmaev I.,
Khamitov I.,
Dodonov S.,
Zhuchkov R.,
Irtuganov E.,
Mescheryakov A.,
Melnikov S.,
Semena A.,
Tkachenko A.,
Aghanim N.,
Sunyaev R. on the optical observations performed previously by our team (Planck Collaboration 2015
a). Data on 13 galaxy
Vertical structure of the outer accretion disk in persistent low-mass X-ray binaries accretion disk in low-mass X-ray binaries by performing
a self-consistent calculation of the vertical
Additional spectroscopic redshift measurements for galaxy clusters from the first Planck catalogueVorobyev V.,
Burenin R.,
Bikmaev I.,
Khamitov I.,
Dodonov S.,
Zhuchkov R.,
Irtuganov E.,
Mescheryakov A.,
Melnikov S.,
Semena A.,
Tkachenko A.,
Aghanim N.,
Sunyaev R. on the optical observations performed previously by our team (Planck Collaboration 2015
a). Data on 13 galaxy
X-ray nova MAXI J1828-249. Evolution of the broadband spectrum during its 2013–2014 outburst, turns out to be moderate during the source’s “high” state (when
a soft blackbody emission component
X-ray nova MAXI J1828-249. Evolution of the broadband spectrum during its 2013–2014 outburst, turns out to be moderate during the source’s “high” state (when
a soft blackbody emission component
New active galactic nuclei among the INTEGRAL and SWIFT X-ray sourcesWe present the results of our optical identifications of
a set of X-ray sources from the INTEGRAL
New active galactic nuclei among the INTEGRAL and SWIFT X-ray sourcesWe present the results of our optical identifications of
a set of X-ray sources from the INTEGRAL