News archive
2011
Galaxies with polar rings (PRGs) are a unique class of extragalactic objects,
consisting of a ring or disk of gas, stars and dust orbiting in a plane
nearly perpendicular to the disk of a central galaxy.
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The results of long-term monitoring of Gigahertz-Peaked Spectrum sources
were found the statistically significant differences (0.05 significance
level) in the high-frequency spectral index distribution between subgroups
of galaxies and quasars.
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According to modern views on the evolution and origin of stars,
most of the stars are members of binary systems. If both
components are massive enough, they eventually go supernova one by
one, whereas their cores collapse, turning into black holes or
neutron stars.
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The history of star formation was successfully analyzed for the first
time based on the spectra of the stellar population of dwarf galaxies
of low surface brightness outside the Local Group.
We have investigated the stellar population of two dwarf spheroidal
galaxies KDG61 and KDG64 in the central part of a close group of
galaxies M81.
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Solar flare activity is produced by the processes of accumulation and
release of energy in an active region. A complex magnetic structure is
formed over the spots, the reconnection of which leads to the generation
of a flare. The information about the magnetic field can be retrieved
from is polarized microwave radiation, the spectrum of which is correlated
with the flare activity.
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As a result of BTA observations of 23 chemically peculiar stars with
strong magnetic fields, it was found that in 22 of them the longitudinal
magnetic field, measured from the hydrogen line cores are considerably
lower (by about 1/3) than the value measured from metal lines in the
same spectra.
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2010
According to the current estimates, a few percent of Main Sequence B5-F5
stars reveal strong surface magnetic fields reaching the values of tens
of kilogauss, which is an order of magnitude greater than the maximal
magnetic field in sunspots.
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The close X-ray binary with relativisic jest, contained probably
a black hole, Cygnus X-3 has been detected in first time
in Gamma-rays at enegries higher 100 ķeV (AGILE, Tavani et al., Nature, 2009)
during the intense radio flares, monitored with RATAN-600 radio telecope.
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By means of deep optical images obtained at the Special Astrophysical
Observatory 6-m telescope it was discovered that some Seyfert galaxies
that were earlier considered to be non-interacting objects displayed
signatures of elongated tidal envelopes belonging to satellite debris.
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CH Cyg is one of the most fascinating as well as the brightest and closest
symbiotic stars. It's composed of an M7 giant and a hot companion, most
likely an accreting white dwarf.
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A bright extended nebulosity around a lenticular galaxy NGC 4460 was
discovered by Igor Karachentsev and Serafim Kaisin (2008, A&A, 479, 603)
during the recent
H

survey of
nearby galaxies on the SAO RAS 6-m telescope.
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In the spectral observations of stars with infrared circular nebulae,
found in the Spitzer survey (24 microns), a new LBV star was discovered
in the Galaxy.
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2009
The brightest of all GRBs known to date, GRB080319B, the "Naked-Eye Burst",
has been observed by our colleagues who acquired its detailed optical light
curve during the stage of gamma emission.
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Dwarf galaxy DDO 68 is the closest to us galaxy (D=10Mpc) with the lowest
metal content known to date. In this galaxy, using the 6 m BTA
telescope, a new massive blue variable star with high luminosity
(>=10
5 Sun's luminocities in visible light) was found.
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New observations of the RC J0311+0507 radio source using the MERLIN
radio interferometer (UK) and the 6-m optical telescope, have added
new strokes to the "portrait" of this unusual object, - one of the most
powerful and distant radio galaxies (z=4.51), and raised new questions
about the origin of the first galaxies in the early Universe.
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A new bright LBV (Luminous Blue Variable) star was found in M33 galaxy.
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The most metal-poor system of four subdwarfs discovered in the solar
neighbourhood.
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Identification and Early Spectroscopic Observations of the Optical
Transient GRB090726.
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Last update: 14/10/2011
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