7,128 research outputs found
The evolution of the jet from Herbig Ae star HD 163296 from 1999 to 2011
Young A and B stars, the so-called Herbig Ae/Be stars (HAeBe), are surrounded
by an active accretion disk and drive outflows. We study the jet HH 409, which
is launched from the HAeBe star HD 163296, using new and archival observations
from Chandra and HST/STIS. In X-rays we can show that the central source is not
significantly extended. The approaching jet, but not the counter-jet, is
detected in Ly alpha. In addition, there is red-shifted Ly alpha emission
extended in the same direction as the jet, that is also absent in the
counter-jet. We can rule out an accretion or disk-wind origin for this feature.
In the optical we find the knots B and B2 in the counter-jet. Knot B has been
observed previously, so we can derive its proper motion of 0.37+-0.01
arcsec/yr. Its electron density is 3000/cm^3, thus the cooling time scale is a
few months only, so the knot needs to be reheated continuously. The shock speed
derived from models of H alpha and forbidden emission lines (FELs) decreased
from 50 km/s in 1999 to 30 km/s in 2011 because the shock front loses energy as
it travels along the jet. Knot B2 is observed at a similar position in 2011 as
knot B was in 1999, but shows a lower ionization fraction and higher mass loss
rate, proving variations in the jet launching conditions.Comment: 14 pages, 8 figures, accepted by A&
Constancy of Expression of the Protein Kinase A Regulatory Subunit Rla in Hepatoma Cell Lines of Different Phenotypes
Higher-order Cartan symmetries in k-symplectic field theory
For k-symplectic Hamiltonian field theories, we study infinitesimal
transformations generated by certain kinds of vector fields which are not
Noether symmetries, but which allow us to obtain conservation laws by means of
a suitable generalization of the Noether theorem.Comment: 11 page
Full-field structured-illumination super-resolution X-ray transmission microscopy
Modern transmission X-ray microscopy techniques provide very high resolution at low and medium X-ray energies, but suffer from a limited field-of-view. If sub-micrometre resolution is desired, their field-of-view is typically limited to less than one millimetre. Although the field-of-view increases through combining multiple images from adjacent regions of the specimen, so does the required data acquisition time. Here, we present a method for fast full-field super-resolution transmission microscopy by structured illumination of the specimen. This technique is well-suited even for hard X-ray energies above 30 keV, where efficient optics are hard to obtain. Accordingly, investigation of optically thick specimen becomes possible with our method combining a wide field-of-view spanning multiple millimetres, or even centimetres, with sub-micron resolution and hard X-ray energies
Chandra observation of Cepheus A: The diffuse emission of HH 168 resolved
X-ray emission from massive stellar outflows has been detected in several
cases. We present a Chandra observation of HH 168 and show that the soft X-ray
emission from a plasma of 0.55 keV within HH 168 is diffuse. The X-ray emission
is observed on two different scales: Three individual, yet extended, regions
are embedded within a complex of low X-ray surface brightness. Compared to the
bow shock the emission is displaced against the outflow direction. We show that
there is no significant contribution from young stellar objects (YSOs) and
discuss several shock scenarios that can produce the observed signatures. We
establish that the X-ray emission of HH 168 is excited by internal shocks in
contrast to simple models, which expect the bow shock to be the most X-ray
luminous.Comment: 8 pages, 5 figures, accepted for publication in A&
Substrate rigidity deforms and polarizes active gels
We present a continuum model of the coupling between cells and substrate that
accounts for some of the observed substrate-stiffness dependence of cell
properties. The cell is modeled as an elastic active gel, adapting recently
developed continuum theories of active viscoelastic fluids. The coupling to the
substrate enters as a boundary condition that relates the cell's deformation
field to local stress gradients. In the presence of activity, the coupling to
the substrate yields spatially inhomogeneous contractile stresses and
deformations in the cell and can enhance polarization, breaking the cell's
front-rear symmetry.Comment: 6 pages, 4 figures, EPL forma
Weak-field limit of Kaluza-Klein models with spherical compactification: experimental constraints
We investigate the classical gravitational tests for the six-dimensional
Kaluza-Klein model with spherical (of a radius ) compactification of the
internal space. The model contains also a bare multidimensional cosmological
constant . The matter, which corresponds to this ansatz, can be
simulated by a perfect fluid with the vacuum equation of state in the external
space and an arbitrary equation of state with the parameter in the
internal space. For example, and correspond to the
monopole two-forms and the Casimir effect, respectively. In the particular case
, the parameter is also absent: . In the
weak-field approximation, we perturb the background ansatz by a point-like
mass. We demonstrate that in the case the perturbed metric
coefficients have the Yukawa type corrections with respect to the usual
Newtonian gravitational potential. The inverse square law experiments restrict
the parameters of the model: $a/\sqrt{\omega_1}\lesssim 6\times10^{-3}\
{{cm}}\gamma\omega_1>0\omega_1=0\gamma=1/3$,
which strongly contradicts the observations.Comment: 8 pages, no figures, revised version, equations and references added,
accepted for publication in Phys. Rev. D. arXiv admin note: significant text
overlap with arXiv:1107.338
Diffraction of a Bose-Einstein condensate from a Magnetic Lattice on a Micro Chip
We experimentally study the diffraction of a Bose-Einstein condensate from a
magnetic lattice, realized by a set of 372 parallel gold conductors which are
micro fabricated on a silicon substrate. The conductors generate a periodic
potential for the atoms with a lattice constant of 4 microns. After exposing
the condensate to the lattice for several milliseconds we observe diffraction
up to 5th order by standard time of flight imaging techniques. The experimental
data can be quantitatively interpreted with a simple phase imprinting model.
The demonstrated diffraction grating offers promising perspectives for the
construction of an integrated atom interferometer.Comment: 4 pages, 4 figure
X-ray to NIR emission from AA Tauri during the dim state - Occultation of the inner disk and gas-to-dust ratio of the absorber
AA Tau is a well-studied, nearby classical T Tauri star, which is viewed
almost edge-on. A warp in its inner disk periodically eclipses the central
star, causing a clear modulation of its optical light curve. The system
underwent a major dimming event beginning in 2011 caused by an extra absorber,
which is most likely associated with additional disk material in the line of
sight toward the central source. We present new XMM-Newton X-ray, Hubble Space
Telescope FUV, and ground based optical and near-infrared data of the system
obtained in 2013 during the long-lasting dim phase. The line width decrease of
the fluorescent H disk emission shows that the extra absorber is located at
au. Comparison of X-ray absorption () with dust extinction (),
as derived from measurements obtained one inner disk orbit (eight days) after
the X-ray measurement, indicates that the gas-to-dust ratio as probed by the
to ratio of the extra absorber is compatible with the ISM ratio.
Combining both results suggests that the extra absorber, i.e., material at
au, has no significant gas excess in contrast to the elevated
gas-to-dust ratio previously derived for material in the inner region
(au).Comment: 16 pages, 12 figures, accepted by A&
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