3,876 research outputs found
The condensin complex is required for proper spindle assembly and chromosome segregation in Xenopus egg extracts.
Chromosome condensation is required for the physical resolution and segregation of sister chromatids during cell division, but the precise role of higher order chromatin structure in mitotic chromosome functions is unclear. Here, we address the role of the major condensation machinery, the condensin complex, in spindle assembly and function in Xenopus laevis egg extracts. Immunodepletion of condensin inhibited microtubule growth and organization around chromosomes, reducing the percentage of sperm nuclei capable of forming spindles, and causing dramatic defects in anaphase chromosome segregation. Although the motor CENP-E was recruited to kinetochores pulled poleward during anaphase, the disorganized chromosome mass was not resolved. Inhibition of condensin function during anaphase also inhibited chromosome segregation, indicating its continuous requirement. Spindle assembly around DNA-coated beads in the absence of kinetochores was also impaired upon condensin inhibition. These results support an important role for condensin in establishing chromosomal architecture necessary for proper spindle assembly and chromosome segregation
M82 - A radio continuum and polarisation study II. Polarisation and rotation measures
The composition and morphology of the interstellar medium in starburst
galaxies has been well investigated, but the magnetic field properties are
still uncertain. The nearby starburst galaxy M82 provides a unique opportunity
to investigate the mechanisms leading to the amplification and reduction of
turbulent and regular magnetic fields. Possible scenarios of the contribution
of the magnetic field to the star-formation rate are evaluated. Archival data
from the VLA and WSRT were combined and re-reduced to cover the wavelength
regime between 3cm and 22cm. All observations revealed polarised emission in
the inner part of the galaxy, while extended polarised emission up to a
distance of 2kpc from the disk was only detected at 18cm and 22cm. The
observations hint at a magnetised bar in the inner part of the galaxy. We
calculate the mass inflow rate due to magnetic stress of the bar to 7.1 solar
masses per year, which can be a significant contribution to the star-formation
rate of M82 of approximately 13 solar masses per year. The halo shows polarised
emission, which might be the remnant of a regular disk field. Indications for a
helical field in the inner part of the outflow cone are provided. The coherence
length of the magnetic field in the centre is similar to the size of giant
molecular clouds. Using polarisation spectra more evidence for a close coupling
of the ionised gas and the magnetic field as well as a two-phase magnetic field
topology were found. Electron densities in the halo are similar to the ones
found in the Milky Way. The magnetic field morphology is similar to the one in
other nearby starburst galaxies with possible large-scale magnetic loops in the
halo and a helical magnetic field inside the outflow cones. The special
combination of a magnetic bar and a circumnuclear ring are able to
significantly raise the star-formation rate in this galaxy by magnetic braking
Heating of solar chromosphere by electromagnetic wave absorption in a plasma slab model
The heating of solar chromospheric inter-network regions by means of the
absorption of electromagnetic (EM) waves that originate from the photospheric
blackbody radiation is studied in the framework of a plasma slab model. The
absorption is provided by the electron-neutral collisions in which electrons
oscillate in the EM wave field and electron-neutral collisions damp the EM
wave. Given the uncertain nature of the collision cross-section due to the
plasma micro-turbulence, it is shown that for plausible physical parameters,
the heating flux produced by the absorption of EM waves in the chromosphere is
between % of the chromospheric radiative loss flux requirement. It is
also established that there is an optimal value for the collision
cross-section, m, that produces the maximal heating
flux of 1990 W m.Comment: Physics of Plasmas, in press, April 2011 issue (final printed
version, typos in proofs corrected
Simple analysis of off-axis solenoid fields using the scalar magnetostatic potential: application to a Zeeman-slower for cold atoms
In a region free of currents, magnetostatics can be described by the Laplace
equation of a scalar magnetic potential, and one can apply the same methods
commonly used in electrostatics. Here we show how to calculate the general
vector field inside a real (finite) solenoid, using only the magnitude of the
field along the symmetry axis. Our method does not require integration or
knowledge of the current distribution, and is presented through practical
examples, including a non-uniform finite solenoid used to produce cold atomic
beams via laser cooling. These examples allow educators to discuss the
non-trivial calculation of fields off-axis using concepts familiar to most
students, while offering the opportunity to introduce important advancements of
current modern research.Comment: 6 pages. Accepted in the American Journal of Physic
- β¦