Ultraluminous X-ray sources in galaxies — microquasars or intermediate mass black holes
S.N. Fabrika a,
P.K. Abolmasov a,
S.V. Karpov a,
O.N. Sholukhova a,
K.K. Ghosh b
a Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Zelenchukskiy Region, Karachai-Cherkessian Republic, Russian Federation
b Universities Space Research Association, NASA Marshall Flight Center, USA
Joint scientific session of the Physical Sciences Division
of the Russian Academy of Sciences
and the Joint Physical Society of the Russian Federation
(30 November 2005)
A joint scientific session of the Physical Sciences Division of
the Russian Academy of Sciences (RAS) and the Joint
Physical Society of the Russian Federation was held in the
Conference Hall of the P N Lebedev Physics Institute, RAS,
on 30 November 2005. The following reports were presented
at the session:
(1) Kuznetsov V D (N V Pushkov Institute of Terrestrial
Magnetism, Ionosphere, and Radio Wave Propagation
(IZMIRAN), RAS, Troitsk, Moscow region) ’Heliophysics:
from observations to models’;
(2) Zaitsev V V (Institute of Applied Physics, RAS,
Nizhnii Novgorod), Stepanov A V (Special Astronomical
Observatory at Pulkovo (GAO), RAS, St.-Petersburg)
’Problems of solar activity physics’;
(3) Churazov E M, Sunyaev R A, Sazonov S Yu,
Revnivtsev M G (Space Research Institute, RAS, Moscow),
Varshalovich D A (A F Ioffe Physical-Technical Institute, RAS, St.-Petersburg) ’Annihilation emission from the galactic center: the INTEGRAL observatory results’;
(4) Fabrika S N, Abolmasov P K, Karpov S V, Sholukhova O N (Special Astrophysical Observatory (SAO),
RAS, Nizhnii Arkhyz, Karachaevo-Cherkesiya Republic),
Ghosh K K (Universities Space Research Association,
NASA Marshall Space Flight Center, USA) ’Ultraluminous X-ray sources in galaxies м microquasars or intermediate mass black holes’.
An abridged version of the reports is given below.
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