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Bow shock and radio halo in the merging cluster A520
M. Markevitch, F. Govoni, G. Brunetti +1
Chandra observations of the merging galaxy cluster A520 reveal a prominent bow shock with M=2.1+0.4-0.3. This is only the second clear example of a substantially supersonic merger…
Constraints on the luminosity of the stellar remnant in SNR1987A
P. Shtykovskiy, A. Lutovinov, M. Gilfanov +1
We obtain photometric constraints on the luminosity of the stellar remnant in SNR1987A using XMM-Newton and INTEGRAL data. The upper limit in the 2--10 keV band based on the XMM-Ne…
Stochastic Dynamics of Magnetosomes in Cytoskeleton
V. N. Binhi, D. S. Chernavskii
Rotations of microscopic magnetic particles, magnetosomes, embedded into the cytoskeleton and subjected to the influence of an ac magnetic field and thermal noise are considered. M…
Gravitational wave experiments and Baksan project "OGRAN"
L. Bezrukov, S. Popov, V. Rudenko +2
A brief sketch of the present status of gravitational wave experiments is given. Attention is concentrated to recent observations with the gravitational detector network. The proje…
X-ray luminosity function of low-mass X-ray binaries in galaxies
K. A. Postnov, A. G. Kuranov
X-ray luminosity function derived from observations of X-ray sources in galactic bulges can be explained by prinicipal evolutionary relations for mass accretion rate onto the compa…
On the Frequency-magnitude Law for Fractal Seismicity
G. Molchan, T. Kronrod
Scaling analysis of seismicity in the space-time-magnitude domain very often starts from the relation N(m,L)=a(L)*10**(-bm)*L**c for the rate of seismic events of magnitude M>m in…