Although for densities and temperatures typical of clusters the gas is optically thin to Thomson scattering for the continuum, ... If there is resonant scattering, ...
INTEGRAL insight into the inner part of the Galaxy. ... Current study (INTEGRAL) Energy band: 20-60 keV ... IGRJ16358-4726 P=5980 22 sec (INTEGRAL, Chandra) ...
XIV Advanced School on Astrophysics Topic III: Observations of the Accretion Disks of Black Holes and Neutron Stars III.3: Accretion Disks of Non-Magnetic Neutron Stars
Paucity of young HMXBs. Popov et al. (1998) (Z=0.02, log(Lmin)=33) ... Paucity of young HMXBs. Evolution of HMXBs population: observational constraints ...
Ni ABUNDANCE IN THE CORE OF THE PERSEUS CLUSTER: AN ANSWER TO THE ... Fabio Gastaldello (CNR-IASF, University of Milan-Bicocca) Silvano Molendi (CNR-IASF) ...
GORU E TEME U ASTROFIZICI Bojan Arbutina Katedra za astronomiju Matemati kog fakulteta Univerziteta u Beogradu arbo@math.rs nere eni problemi u astrofizici gama ...
Excitation of the Neutron Star f-mode in LMXBs. J. C. N. de Araujo, O. D. Miranda & O. D. Aguiar ... the glitch phenomenon (see de Araujo, Miranda & Aguiar 2005) ...
General motivation for extragalactic studies. More objects. Cleaner star formation history ... Emission resolved & luminosity functions measured (Sarazin, Irwin ...
High Energy Universe Viewed Through Astrosat P.C.Agrawal Tata Institute of Fundamental Research, Mumbai Talk at the Chandrayan Symposium at IMSc , Chennai , January 4 ...
(Towards) A unified model of X-ray variability in X-ray binaries and AGN. Phil ... L(t) has a Gaussian distribution, so X(t) has a lognormal distribution...
NGC 821: high resolution & long exposures. Isolated E galaxy with old stellar population ... High-resolution imaging, sensitive, time-monitoring. Light-curves, XLFs ...