Anisotropic distribution functions for spherical galaxiesA method is presented for finding anisotropic distribution functions for stellar systems with known, spherically symmetric, densities, which depends only on the two classical integrals of the energy…Zhenglu Jiang, Leonid Ossipkov·Dec 29, 2008SaveLearn
Quantum vacuum and accelerated expansionA new approach to extraction of quantum vacuum energy, in the context of the accelerated expansion, is proposed, and it is shown that experimentally realistic orders of values can be derived. The…Bogusław Broda, Michał Szanecki·Dec 29, 2008SaveLearn
Near-IR spectroscopic ages of massive star clusters in M82Like other starburst galaxies, M82 hosts compact, massive young star clusters that are interesting both in their own right and as benchmarks for population synthesis models. Can spectral synthesis…A. Lançon, J. S. Gallagher, M. Mouhcine et al.·Dec 29, 2008SaveLearn
Infall and rotation motions in the HH 111 protostellar system: A flattened envelope in transition to a disk?We have mapped the central region of the HH 111 protostellar system in 1.33 mm continuum, C18O(J=2-1), 13CO (J=2-1), and SO (NJ=56-45) emission at ~3" resolution with the Submillimeter Array.…Chin-Fei Lee, Yao-Yuan Mao, Bo Reipurth·Dec 29, 2008SaveLearn
Angular Energy Distribution of Collapsar-JetsCollapsars are fast-spinning, massive stars, whose core collapse liberates an energy, that can be channeled in the form of ultrarelativistic jets. These jets transport the energy from the collapsed…Akira Mizuta, Miguel A. Aloy·Dec 28, 2008SaveLearn
Jet breaks and Energetics of Swift GRB X-ray AfterglowsWe present a systematic temporal and spectral study of all Swift-XRT observations of GRB afterglows discovered between 2005 January and 2007 December. After constructing and fitting all light curves…J. L. Racusin, E. W. Liang, D. N. Burrows et al.·Dec 28, 2008SaveLearn
Orbital resonances in discs around braneworld Kerr black holesRotating black holes in the brany universe of the Randall-Sundrum type are described by the Kerr geometry with a tidal charge b representing the interaction of the brany black hole and the bulk…Zdenek Stuchlik, Andrea Kotrlova·Dec 28, 2008SaveLearn
Dynamic masses for the close PG1159 binary SDSSJ212531.92-010745.9SDSSJ212531.92-010745.9 is the first known PG1159 star in a close binary with a late main sequence companion allowing a dynamical mass determination. The system shows flux variations with a…S Schuh, B Beeck, T Nagel·Dec 28, 2008SaveLearn
Long-term photometric monitoring of the hybrid subdwarf B pulsator HS0702+6043Pulsating subdwarf B stars oscillate in short-period p-modes or long-period g-modes. HS 0702 + 6043 is one of currently three objects known to show characteristics of both types and hence is…R. Lutz, S. Schuh, R. Silvotti et al.·Dec 28, 2008SaveLearn
Spectroscopy of the sdB pulsator HS2201+2610We present time resolved echelle spectra of the planet-hosting subdwarf B pulsator HS 2201 + 2610 and report on our efforts to extract pulsational radial velocity measurements from this data.R. Kruspe, S. Schuh, R. Silvotti et al.·Dec 28, 2008SaveLearn
Multi-wavelength photometric variation of PG1605+072In a large coordinated attempt to further our understanding of the p-mode pulsating sdB star PG1605+072, the Multi-Site Spectroscopic Telescope (MSST) collaboration has obtained simultaneous…S. Schuh, S. Dreizler, U. Heber et al.·Dec 28, 2008SaveLearn
Dark Stars: the First Stars in the Universe may be powered by Dark Matter HeatingA new line of research on Dark Stars is reviewed, which suggests that the first stars to exist in the universe were powered by dark matter heating rather than by fusion. Weakly Interacting Massive…Katherine Freese, Peter Bodenheimer, Paolo Gondolo et al.·Dec 28, 2008SaveLearn
PIERNIK mhd code - a multi-fluid, non-ideal extension of the relaxing-TVD scheme (III)We present a new multi-fluid, grid MHD code PIERNIK, which is based on the Relaxing TVD scheme (Jin & Xin, 1995). The original scheme (see Trac & Pen (2003) and Pen et al. (2003)) has been extended…Michał Hanasz, Kacper Kowalik, Dominik Wóltański et al.·Dec 28, 2008SaveLearn
The variation of the electromagnetic coupling and quintessenceThe properties of quintessence are examined through the study of the variation of the electromagnetic coupling. We consider two simple quintessence models with a modified exponential potential and…M. C. Bento, R. Gonzalez Felipe·Dec 28, 2008SaveLearn
3D Spectroscopic Study of the Line Emitting Regions of Mrk 493We report the results of 3D spectroscopic observations of Mrk 493 (NLS1 galaxy) with the integral-field spectrograph MPFS of the SAO RAS 6-m telescope. The difference in the slope of the optical…L. C. Popovic, A. A. Smirnova, J. Kovacevic et al.·Dec 28, 2008SaveLearn
Explosions inside Ejecta and Most Luminous SupernovaeThe extremely luminous supernova SN2006gy is explained in the same way as other SNIIn events: light is produced by a radiative shock propagating in a dense circumstellar envelope formed by a previous…S. I. Blinnikov·Dec 28, 2008SaveLearn
Quasi-viscous accretion flow -- I: Equilibrium conditions and asymptotic behaviourIn a novel approach to studying viscous accretion flows, viscosity has been introduced as a perturbative effect, involving a first-order correction in the α-viscosity parameter. This method reduces…Jayanta K. Bhattacharjee, Atri Bhattacharya, Tapas K. Das et al.·Dec 28, 2008SaveLearn
Observations of the pulsation of the Cepheid l Car with the Sydney University Stellar InterferometerObservations of the southern Cepheid l Car to yield the mean angular diameter and angular pulsation amplitude have been made with the Sydney University Stellar Interferometer (SUSI) at a wavelength…J. Davis, A. P. Jacob, J. G. Robertson et al.·Dec 28, 2008SaveLearn
Reversal of the amplitude difference of kHz QPOs in six atoll sourcesAIMS: For six neutron-star atoll sources (4U 1608-52, 4U 1636-53, 4U 0614+09, 4U 1728-34, 4U 1820-30 and 4U 1735-44) we investigate the relationship between the observed fractional rms amplitudes of…Gabriel Torok·Dec 27, 2008SaveLearn
The origin of 'Great Walls'A new semianalytical model that explains the formation and sizes of the 'great walls' - the largest structures observed in the universe is suggested. Although the basis of the model is the…Sergei Shandarin·Dec 27, 2008SaveLearn
Thermal axion constraints in non-standard thermal historiesThere is no direct evidence for radiation domination prior to big-bang nucleosynthesis, and so it is useful to consider how constraints to thermally-produced axions change in non-standard thermal…Daniel Grin, Tristan Smith, Marc Kamionkowski·Dec 27, 2008SaveLearn
Constraints on Dark Energy from the Observed Expansion of our Cosmic HorizonWithin the context of standard cosmology, an accelerating universe requires the presence of a third `dark' component of energy, beyond matter and radiation. The available data, however, are still…Fulvio Melia·Dec 27, 2008SaveLearn
Realistic analytic model for the prompt and high latitude emission in GRBsMost gamma-ray bursts (GRBs) observed by the Swift satellite show an early rapid decay phase (RDP) in their X-ray lightcurve, which is usually a smooth continuation of the prompt gamma-ray emission,…F. Genet, J. Granot·Dec 26, 2008SaveLearn
Rapid pulsations in sub-THz solar burstsA new solar burst emission spectral component has been found showing sub-THz fluxes increasing with frequency, spectrally separated from the well known microwave component. Rapid pulsations are found…Pierre Kaufmann, C. Guillermo Gimenez de Castro, Emilia Correia et al.·Dec 26, 2008SaveLearn
Photometric Properties of the Near-contact Binary GW GeminorumNew multiband CCD photometry is presented for the eclipsing binary GW Gem; the RI light curves are the first ever compiled. Four new minimum timings have been determined. Our analysis of eclipse…Jae Woo Lee, Seung-Lee Kim, Chung-Uk Lee et al.·Dec 25, 2008SaveLearn