41,374 research outputs found
Morphology-dependent trends of galaxy age with environment in Abell 901/902 seen with COMBO-17
We investigate correlations between galaxy age and environment in the Abell
901/2 supercluster for separate morphologies. Using COMBO-17 data, we define a
sample of 530 galaxies, complete at on an area of (Mpc/). We explore several age indicators including an
extinction-corrected residual from the colour-magnitude relation (CMR). As a
result, we find a clear trend of age with density for galaxies of all
morphologies that include a spheroidal component, in the sense that galaxies in
denser environments are older. This trend is not seen among Scd/Irr galaxies
since they all have young ages. However, the trend among the other types is
stronger for fainter galaxies. While we also see an expected age-morphology
relation, we find no evidence for a morphology-density relation at fixed age.Comment: Accepted for publication in MNRAS (Letters
The effect of stellar feedback on the formation and evolution of gas and dust tori in AGN
Recently, the existence of geometrically thick dust structures in Active
Galactic Nuclei (AGN) has been directly proven with the help of mid-infrared
interferometry. The observations are consistent with a two-component model made
up of a geometrically thin and warm central disk, surrounded by a colder,
fluffy torus component. In an exploratory study, we investigate one possible
physical mechanism, which could produce such a structure, namely the effect of
stellar feedback from a young nuclear star cluster on the interstellar medium
in centres of AGN. The model is realised with the help of the hydrodynamics
code TRAMP. We follow the evolution of the interstellar medium by taking
discrete mass loss and energy ejection due to stellar processes, as well as
optically thin radiative cooling into account. In a post-processing step, we
calculate observable quantities (spectral energy distributions and images) with
the help of the radiative transfer code MC3D. The interplay between injection
of mass, supernova explosions and radiative cooling leads to a two-component
structure made up of a cold geometrically thin, but optically thick and very
turbulent disk residing in the vicinity of the angular momentum barrier,
surrounded by a filamentary structure. The latter consists of cold long radial
filaments flowing towards the disk and a hot tenuous medium in between, which
shows both inwards and outwards directed motions. This modelling is able to
reproduce the range of observed neutral hydrogen column densities of a sample
of Seyfert galaxies as well as the relation between them and the strength of
the silicate 10 micron spectral feature. Despite being quite crude, our mean
Seyfert galaxy model is even able to describe the SEDs of two intermediate type
Seyfert galaxies observed with the Spitzer Space Telescope.Comment: 16 pages, 11 figures, accepted by MNRAS, high resolution version can
be downloaded from:
http://www.mpe.mpg.de/~mschartm/papers/schartmann_2008b.pd
Supersymmetric features of the Maxwell fish-eye lens
We provide a supersymmetric analysis of the Maxwell fisheye (MF) wave problem
at zero energy. Working in the so-called sector, we obtain the
corresponding superpartner (fermionic) MF effective potential within Witten's
one-dimensional (radial) supersymmetric procedure.Comment: 5 pages in Latex, one figure not included has been published as Fig.
2 in Phys. Lett. A 208 (1995) 33-3
Evidence for multiple superconducting gaps in optimally doped BaFeCoAs from infrared spectroscopy
We performed combined infrared reflection and ellipsometry measurements of
the in-plane optical reponse of single crystals of the pnictide high
temperature superconductor BaFeCoAs with = 24.5
K. We observed characteristic superconductivity-induced changes which provide
evidence for at least three different energy gaps. We show that a BCS-model of
isotropic gaps with 2 of 3.1, 4.7, and 9.2 reproduces the
experimental data rather well. We also determine the low-temperature value of
the in-plane magnetic penetration depth of 270 nm
Baryonic contributions to the dilepton spectrum of nucleon-nucleon collisions
We study the production of dileptons in relativistic nucleon-nucleon
collisions. Additionally to the traditional dilepton production channels
(vector meson decays, meson and Delta(1232) Dalitz decays) we included in our
model as new dilepton sources the Dalitz decay of higher unflavored baryon
resonances with spin<=5/2 and mass<=2.25 GeV/c^2. The contributions of these
new channels are estimated using experimental information about the Ngamma
decays of the resonances and have large uncertainties. The obtained dilepton
spectra are compared to the experimental data by the DLS collaboration.
Predictions for the HADES detector (SIS, GSI) are also discussed. In spite of
the large uncertainties of the higher resonance Dalitz decay contributions we
are able to draw the conclusion that these contributions are negligible
compared to the other dilepton sources and do not influence the detectability
of the phi and omega vector meson peaks.Comment: 9 pages, 4 figures, version accepted for publication in Phys. Rev.
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