4,082 research outputs found
The portrait of Malin 2: a case study of a giant low surface brightness galaxy
The low surface brightness disc galaxy Malin2 challenges the standard theory
of galaxy evolution by its enormous total mass ~2 10^12 Ms which must have been
formed without recent major merger events. The aim of our work is to create a
coherent picture of this exotic object by using the new optical multicolor
photometric and spectroscopic observations at Apache Point Observatory as well
as archival datasets from Gemini and wide-field surveys. We performed the
Malin2 mass modelling, estimated the contribution of the host dark halo and
found that it had acquired its low central density and the huge isothermal
sphere core radius before the disc subsystem was formed. Our spectroscopic data
analysis reveals complex kinematics of stars and gas in the very inner region.
We measured the oxygen abundance in several clumps and concluded that the gas
metallicity decreases from the solar value in the centre to a half of that at
20-30 kpc. We found a small satellite and measured its mass (1/500 of the host
galaxy) and gas metallicity. One of the unique properties of Malin2 turned to
be the apparent imbalance of ISM: the molecular gas is in excess with respect
to the atomic gas for given values of the gas equilibrium turbulent pressure.
We explain this imbalance by the presence of a significant portion of the dark
gas not observable in CO and the Hi 21 cm lines. We also show that the
depletion time of the observed molecular gas traced by CO is nearly the same as
in normal galaxies. Our modelling of the UV-to-optical spectral energy
distribution favours the exponentially declined SFH over a single-burst
scenario. We argue that the massive and rarefied dark halo which had formed
before the disc component well describes all the observed properties of Malin2
and there is no need to assume additional catastrophic scenarios proposed
previously to explain the origin of giant LSB galaxies. [Abbreviated]Comment: 17 pages, 10 figures, accepted for publication in MNRA
Relaxation time spectrum of low-energy excitations in one- and two-dimensional materials with charge or spin density waves
The long-time thermal relaxation of (TMTTF)Br, SrCuO
and SrCaCuO single crystals at temperatures below 1 K
and magnetic field up to 10 T is investigated. The data allow us to determine
the relaxation time spectrum of the low energy excitations caused by the
charge-density wave (CDW) or spin-density wave (SDW). The relaxation time is
mainly determined by a thermal activated process for all investigated
materials. The maximum relaxation time increases with increasing magnetic
field. The distribution of barrier heights corresponds to one or two Gaussian
functions. The doping of SrCaCuO with Ca leads to
a drastic shift of the relaxation time spectrum to longer time. The maximum
relaxation time changes from 50 s (x = 0) to 3000 s (x = 12) at 0.1 K and 10 T.
The observed thermal relaxation at x=12 clearly indicates the formation of the
SDW ground state at low temperatures
Lie symmetry analysis and exact solutions of the quasi-geostrophic two-layer problem
The quasi-geostrophic two-layer model is of superior interest in dynamic
meteorology since it is one of the easiest ways to study baroclinic processes
in geophysical fluid dynamics. The complete set of point symmetries of the
two-layer equations is determined. An optimal set of one- and two-dimensional
inequivalent subalgebras of the maximal Lie invariance algebra is constructed.
On the basis of these subalgebras we exhaustively carry out group-invariant
reduction and compute various classes of exact solutions. Where possible,
reference to the physical meaning of the exact solutions is given. In
particular, the well-known baroclinic Rossby wave solutions in the two-layer
model are rediscovered.Comment: Extended version, 24 pages, 1 figur
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