CNO driven winds of hot first starsDuring the evolution of first stars, the CNO elements may emerge on their surfaces due to the mixing processes. Consequently, these stars may have winds driven purely by CNO elements. We study the…Jiri Krticka, Jiri Kubat·Oct 16, 2008SaveLearn
Deceleration of arbitrarily magnetized GRB ejecta: the complete evolution(Abridged) We aim to quantitatively understand the dynamical effect and observational signatures of magnetization of the GRB ejecta on the onset of the afterglow. We perform ultrahigh-resolution…P. Mimica, D. Giannios, M. A. Aloy·Oct 16, 2008SaveLearn
Prompt GeV Emission from Residual Collisions in GRB Outflows: Evidence from Fermi Observations of GRB 080916cThe gamma-rays from gamma-ray bursts (GRBs) are believed to be produced by internal shocks driven by small timescale, ~1 ms, variation in the GRB outflows, and a pair-production spectral cutoff is…Zhuo Li·Oct 16, 2008SaveLearn
Testing Inflation: A Bootstrap ApproachWe note that the essential idea of inflation, that the universe underwent a brief period of accelerated expansion followed by a long period of decelerated expansion, can be encapsulated in a…Latham Boyle, Paul J. Steinhardt·Oct 16, 2008SaveLearn
Galactic and Extragalactic Magnetic FieldsThe strength of the total magnetic field in our Milky Way from radio Zeeman and synchrotron measurements is about 6 muG near the Sun and several mG in dense clouds, pulsar wind nebulae, and filaments…Rainer Beck·Oct 16, 2008SaveLearn
Dust Extinction in High-z Galaxies with GRB Afterglow Spectroscopy - The 2175Å Feature at z=2.45We report the clear detection of the 2175A dust absorption feature in the optical afterglow spectrum of the gamma-ray burst (GRB) GRB070802 at a redshift of z=2.45. This is the highest redshift for a…Á. Elíasdóttir, J. P. U. Fynbo, J. Hjorth et al.·Oct 16, 2008SaveLearn
Gamma-ray burst afterglows : luminosity clustering at infrared wavelengths?Clustering in the luminosity of the afterglows of gamma-ray burst has been reported in the optical and X-ray. We investigate the possibility that a clustering in the luminosity of the afterglows of…B. Gendre, S. Pelisson, M. Boer et al.·Oct 16, 2008SaveLearn
Discovery of a very highly extinguished supernova in a luminous infrared galaxyWe report the discovery of a confirmed supernova (SN) and a supernova-candidate in near-infrared images from the ALTAIR/NIRI adaptive optics system on the Gemini-North Telescope and NICMOS on the…E. Kankare, S. Mattila, S. Ryder et al.·Oct 16, 2008SaveLearn
Forbush decreases and turbulence levels at CME frontsWe seek to estimate the average level of MHD turbulence near coronal mass ejection (CME) fronts as they propagate from the Sun to the Earth. We examine the cosmic ray data from the GRAPES-3 tracking…Prasad Subramanian, H. M. Antia, S. R. Dugad et al.·Oct 16, 2008SaveLearn
Influence of Dark Matter on Light Propagation in Solar SystemWe investigated the influence of dark matter on light propagation in the solar system. We assumed the spherical symmetry of spacetime and derived the approximate solution of the Einstein equation,…Hideyoshi Arakida·Oct 16, 2008SaveLearn
Spitzer Spectral Mapping of Supernova Remnant Cassiopeia AWe present the global distribution of fine structure infrared line emission in the Cassiopeia A supernova remnant using data from the Spitzer Space Telescope's Infrared Spectrograph. We identify…J. D. T. Smith, Lawrence Rudnick, Tracey Delaney et al.·Oct 16, 2008SaveLearn
A Universal Central Engine Hypothesis for Short and Long GRBsIt is noted that X-ray tails (XRTs) of short, hard γ-ray bursts (SHBs) are similar to X-ray flashes (XRFs). We suggest a universal central engine hypothesis, as a way of accounting for this…David Eichler, Dafne Guetta, Hadar Manis·Oct 16, 2008SaveLearn
Spectroscopic Constraints on (pseudo-)Scalar Particles from Compact Astrophysical ObjectsWe propose a new method to search for light (pseudo-)scalar particles in the spectra of compact astrophysical objects such as magnetars, pulsars, and quasars. On accounts of compact astrophysical…Doron Chelouche, Raul Rabadan, Sergey Pavlov et al.·Oct 16, 2008SaveLearn
Compact groups in theory and practice - II. Comparing the observed and predicted nature of galaxies in compact groupsWe examine the properties of galaxies in compact groups identified in a mock galaxy catalogue based upon the Millennium Run simulation. The overall properties of groups identified in projection are…Crystal M. Brasseur, Alan W. McConnachie, Sara L. Ellison et al.·Oct 16, 2008SaveLearn
Spectral Lags Explained as Scattering from Accelerated ScatterersA quantitative theory of spectral lags for γ-ray bursts (GRBs) is given. The underlying hypothesis is that GRB subpulses are photons that are scattered into our line of sight by local…David Eichler, Hadar Manis·Oct 16, 2008SaveLearn
First Results from the Lick AGN Monitoring Project: The Mass of the Black Hole in Arp 151We have recently completed a 64-night spectroscopic monitoring campaign at the Lick Observatory 3-m Shane telescope with the aim of measuring the masses of the black holes in 13 nearby (z < 0.05)…Misty C. Bentz, Jonelle L. Walsh, Aaron J. Barth et al.·Oct 16, 2008SaveLearn
Cosmic Analogues of the Stern-Gerlach Experiment and the Detection of Light BosonsWe show that, by studying the arrival times of radio pulses from highly-magnetized pulsars, it may be possible to detect light spin-0 bosons (such as axions and axion-like particles) with a much…Doron Chelouche, Eduardo I. Guendelman·Oct 16, 2008SaveLearn
Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical ObservationsIt has been claimed that Period-Luminosity relations derived from infrared observations of Large Magellanic Cloud (LMC) Cepheids are less dependent on the metallicity of the Cepheids. In this work,…Hilding R. Neilson, Chow-Choong Ngeow, Shashi M. Kanbur et al.·Oct 16, 2008SaveLearn
On Flare Driven Global WavesWe recently presented evidence of a strong correlation between the energy in the high-frequency part of the acoustic spectrum of the Sun and the solar X-ray flux Karoff & Kjeldsen (2008). The…C. Karoff·Oct 16, 2008SaveLearn
High-resolution molecular line observations of active galaxiesThe study of the content, distribution and kinematics of interstellar gas is a key to understand the origin and maintenance of both starburst and nuclear (AGN) activity in galaxies. The processes…S. Garcia-Burillo, F. Combes, A. Usero et al.·Oct 16, 2008SaveLearn
Prospects for Studies of Stellar Evolution and Stellar Death in the JWST EraI review the prospects for studies of the advanced evolutionary stages of low-, intermediate- and high-mass stars by the JWST and concurrent facilities, with particular emphasis on how they may help…Michael J. Barlow·Oct 16, 2008SaveLearn
High variability in Vela X-1: giant flares and off statesWe investigate the spectral and temporal behavior of the high mass X-ray binary Vela X-1 during a phase of high activity, with special focus on the observed giant flares and off states. INTEGRAL…Ingo Kreykenbohm, Joern Wilms, Peter Kretschmar et al.·Oct 16, 2008SaveLearn
Pair-Starved Pulsar MagnetospheresWe propose a simple analytic model for the innermost (within the light cylinder of canonical radius) structure of open-magnetic-field lines of a rotating neutron star (NS) with relativistic outflow…Alex G. Muslimov, Alice K. Harding·Oct 16, 2008SaveLearn
The Elemental Composition of High-Energy Cosmic Rays: Measurements with TRACERTRACER ('Transition Radiation Array for Cosmic Energetic Radiation') is a balloon borne instrument that has been developed to directly measure the composition and energy spectra of individual…P. J. Boyle·Oct 16, 2008SaveLearn
Revisiting the theoretical DBV (V777 Her) instability strip: the MLT theory of convectionWe reexamine the theoretical instability domain of pulsating DB white dwarfs (DBV or V777 Her variables). We performed an extensive g-mode nonadiabatic pulsation analysis of DB evolutionary models…A. H. Córsico, L. G. Althaus, M. M. Miller Bertolami et al.·Oct 16, 2008SaveLearn