A hydrodynamic model for asymmetric explosions of rapidly rotating collapsing supernovae with a toroidal atmosphereAstronomy Letters - Tập 30 - Trang 803-815 - 2004
V. S. Imshennik, K. V. Manukovskii
We numerically solved the two-dimensional axisymmetric hydrodynamic problem of
the explosion of a low-mass neutron star in a circular orbit. In the initial
conditions, we assumed a nonuniform density distribution in the space
surrounding the collapsed iron core in the form of a stationary toroidal
atmosphere that was previously predicted analytically and computed numerically.
The configuration of ... hiện toàn bộ
Models of Magnetospheric Accretion onto Young Stars in the Absence of Ionization EquilibriumAstronomy Letters - Tập 48 - Trang 29-37 - 2022
D. V. Dmitriev, V. P. Grinin
The formation of hydrogen emission lines in the magnetospheres of young stars is
considered. The magnetosphere is assumed to be formed by a dipole magnetic field
whose axis is aligned with the stellar rotation axis. The radiative transfer in
spectral lines is considered in the Sobolev approximation with nonlocal
radiative coupling. We have taken into account the effect of gas ionization
fraction t... hiện toàn bộ
Photometric observations of Cepheids from the ASAS-3 catalog: Photoelectric BV I c observations of 46 low-amplitude CepheidsAstronomy Letters - Tập 35 - Trang 311-320 - 2009
L. N. Berdnikov, A. Yu. Kniazev, V. V. Kravtsov, E. N. Pastukhova, D. G. Turner
From December 2006 to January 2008, we performed 1699 BV I c observations for 46
low-amplitude Cepheids discovered in the course of the ASAS project using the
76-cm telescope of the South-African Astronomical Observatory (SAAO). We provide
the tables of observations and V light and B-V and V-I c color curves. These new
observations, along with data from the ASAS-3 catalog, have been used to improv... hiện toàn bộ
Fine core-jet structure of the galaxy M87Astronomy Letters - Tập 37 - Trang 154-170 - 2011
L. I. Matveyenko, S. V. Seleznev
The fine core-jet structure of the radio galaxy M87 has been investigated in the
millimeter-decimeter wave band. A counterjet whose extent is ρ(λ) ≈ 0.036λ pc,
where the wavelength λ is expressed in centimeters, has been identified. At a
wavelength of 2 cm, the brightness of the jet and counterjet decreases
exponentially to the minimally detectable level. However, the decline for the
jet slows dow... hiện toàn bộ
New Estimates of the Merger Rate of Primordial Black Holes with Allowance for Clustering Dark MatterAstronomy Letters - Tập 48 - Trang 561-567 - 2023
M. V. Tkachev, S. V. Pilipenko
The merger rate of primordial black holes (PBHs) is numerically estimated by
taking into account the gravitational interaction of PBHs with clustering cold
dark matter (DM). The mass and initial separation have values appropriate for
the explanation of LIGO/Virgo events by the merging of binary PBHs. We refine
the criterion for the merging of a pair of black holes, provided that a DM halo
is forme... hiện toàn bộ
The soft X-ray novae, black-hole candidates XTE J2012+381 and XTE J 1550-564Astronomy Letters - Tập 28 - Trang 660-668 - 2002
N. L. Aleksandrovich, V. A. Aref'ev
In 1998–1999, the X-ray transients XTE J2012+381 and XTE J1550-564 were observed
with the TTM X-ray telescope onboard the Mir-Kvant astrophysical module.
Spectral properties of these sources on the descent of the light curve after the
secondary maxima of their outbursts are studied. Upper limits on the off-state
flux are given. Comparison with other X-ray novae observed with the TTM
telescope lead... hiện toàn bộ