34,030 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
Energy Gap from Tunneling and Metallic Sharvin Contacts onto MgB2: Evidence for a Weakened Surface Layer
Point-contact tunnel junctions using a Au tip on sintered MgB2 pellets reveal
a sharp superconducting energy gap that is confirmed by subsequent metallic
Sharvin contacts made on the same sample. The peak in the tunneling conductance
and the Sharvin contact conductance follow the BCS form, but the gap values of
4.3 meV are less than the weak-coupling BCS value of 5.9 meV for the bulk Tc of
39 K. The low value of Delta compared to the BCS value for the bulk Tc is
possibly due to chemical reactions at the surface.Comment: 3 pages, 3 figure
Experimental Investigations of Elastic Tail Propulsion at Low Reynolds Number
A simple way to generate propulsion at low Reynolds number is to periodically
oscillate a passive flexible filament. Here we present a macroscopic
experimental investigation of such a propulsive mechanism. A robotic swimmer is
constructed and both tail shape and propulsive force are measured. Filament
characteristics and the actuation are varied and resulting data are
quantitatively compared with existing linear and nonlinear theories
Probing the Phase Diagram of Bi2Sr2CaCu2O8+d with Tunneling Spectroscopy
Tunneling measurements are performed on Ca-rich single crystals of
Bi2Sr2CaCu2O8+d (Bi2212), with various oxygen doping levels, using a novel
point contact method. At 4.2 K, SIN and SIS tunnel junctions are obtained with
well-defined quasiparticle peaks, robust dip and hump features and in some
cases Josephson currents. The doping dependence of tunneling conductances of
Ca-rich Bi2212 are analyzed and compared to stoichiometric Bi2212. A similar
profile of energy gap vs. doping concentration is found although the Ca-rich
samples have a slighly smaller optimum Tc and therefore smaller gap values for
any doping level. The evolution of tunneling conductance peak height to
background ratios with hole concentration are compared. For a given doping
level, the Ca-rich spectra showed more broadened features compared to the
stoichiometric counterparts, most likely due to increased disorder from the
excess Ca. Comparison of the dip and hump features has provided some potential
insights into their origins.Comment: 4 pages, 4 figures; presented at the Applied Superconductivity
Conference (August 4-9, 2002) in Houston, TX; to be published in IEEE Trans.
Appl. Supercon
Environmental dependence of AGN activity in the supercluster A901/2
We present XMM data for the supercluster A901/2, at z ~ 0.17, which is
combined with deep imaging and 17-band photometric redshifts (from the COMBO-17
survey), 2dF spectra and Spitzer 24um data, to identify AGN in the
supercluster. The 90ksec XMM image contains 139 point sources, of which 11 are
identified as supercluster AGN with L_X(0.5-7.5keV) > 1.7x10^41 erg/cm2/s. The
host galaxies have M_R < -20 and only 2 of 8 sources with spectra could have
been identified as AGN by the detected optical emission lines. Using a large
sample of 795 supercluster galaxies we define control samples of massive
galaxies with no detected AGN. The local environments of the AGN and control
samples differ at >98 per cent significance. The AGN host galaxies lie
predominantly in areas of moderate projected galaxy density and with more local
blue galaxies than the control sample, with the exception of one very bright
Type I AGN very near the centre of a cluster. These environments are similar
to, but not limited to, cluster outskirts and blue groups. Despite the large
number of potential host galaxies, no AGN are found in regions with the highest
galaxy density (excluding some cluster cores where emission from the ICM
obscures moderate luminosity AGN). AGN are also absent from the areas with
lowest galaxy density. We conclude that the prevalence of cluster AGN is linked
to their environment.Comment: 20 pages, 15 figures. MNRAS accepted. Version with full resolution
figures, including Figure 14, is available at
http://www.sc.eso.org/~rgilmour
Discovery of a Non-Thermal Galactic Center Filament (G358.85+0.47) Parallel to the Galactic Plane
We report the discovery of a new non-thermal filament, G358.85+0.47, the
``Pelican'', located ~225 pc in projection from SgrA, and oriented parallel to
the Galactic plane. VLA continuum observations at 20 cm reveal that this 7'
(17.5 pc) structure bends at its northern extension and is comprised of
parallel strands, most apparent at its ends. Observations at 6 and 3.6 cm
reveal that the Pelican is a synchrotron-emitting source and is strongly
linearly polarized over much of its extent. The spectral index of the filament
changes from alpha(20/6)=-0.8 to alpha(6/3.6)=-1.5. The rotation measures
exhibit a smooth gradient, with values ranging from -1000 rad/m2 to +500
rad/m2. The intrinsic magnetic field is well-aligned along the length of the
filament. Based on these properties, we classify the Pelican as one of the
non-thermal filaments unique to the Galactic center. Since these filaments
(most of which are oriented perpendicular to the Galactic plane) are believed
to trace the overall magnetic field in the inner Galaxy, the Pelican is the
first detection of a component of this field parallel to the plane. The Pelican
may thus mark a transition region of the magnetic field orientation in the
inner kiloparsec of the Galaxy.Comment: 6 pages, 4 figures, to appear in ApJ Letters; Figs. 2 & 3 are color
.ps files and best viewed in colo
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