Luminosity of a quark star undergoing torsional oscillations and the problem of gamma ray burstsWe discuss whether the winding-up of the magnetic field by differential rotation in a new-born quark star can produce a sufficiently-high, energy, emission rate of sufficiently long duration to…J. Heyvaerts, S. Bonazzola, M. Bejger et al.·Nov 7, 2008SaveLearn
Measurement of acoustic properties of South Pole ice for neutrino astronomySouth Pole ice is predicted to be the best medium for acoustic neutrino detection. Moreover, ice is the only medium in which all three dense-medium detection methods (optical, radio, and acoustic)…Justin Vandenbroucke·Nov 7, 2008SaveLearn
Translational Invariance and the Anisotropy of the Cosmic Microwave BackgroundPrimordial quantum fluctuations produced by inflation are conventionally assumed to be statistically homogeneous, a consequence of translational invariance. In this paper we quantify the potentially…Sean M. Carroll, Chien-Yao Tseng, Mark B. Wise·Nov 7, 2008SaveLearn
Prompt GeV emission in the synchrotron self-Compton model for Gamma-Ray BurstsThe detection in 10 bursts of an optical counterpart emission (i.e. during the prompt GRB phase) that is 10-10000 brighter than the extrapolation of the burst spectrum to optical frequencies suggests…A. Panaitescu·Nov 7, 2008SaveLearn
A Photometrically and Morphologically Variable Infrared Nebula in L483We present narrow and broad K-band observations of the Class 0/I source IRAS 18148-0440 that span 17 years. The infrared nebula associated with this protostar in the L483 dark cloud is both…Michael Connelley, Klaus Hodapp, Gary Fuller·Nov 7, 2008SaveLearn
Photometry and Spin Rate Distribution of Small-Sized Main Belt AsteroidsPhotometry results of 32 asteroids are reported from only seven observing nights on only seven fields, consisting of 34.11 cumulative hours of observations. The data were obtained with a wide-field…D. Polishook, N. Brosch·Nov 7, 2008SaveLearn
Uncertainties in Theoretical HeI Emissivities: HII Regions, Primordial Abundance, and Cosmological RecombinationA number of recent works in astronomy and cosmology have relied upon theoretical He I emissivities, but we know of no effort to quantify the uncertainties in the atomic data. We analyze and assign…R. L. Porter, G. J. Ferland, K. B. MacAdam et al.·Nov 7, 2008SaveLearn
Bayesian modelling of clusters of galaxies from multi-frequency pointed Sunyaev--Zel'dovich observationsWe present a Bayesian approach to modelling galaxy clusters using multi-frequency pointed observations from telescopes that exploit the Sunyaev--Zel'dovich effect. We use the recently developed…F. Feroz, M. P. Hobson, J. T. L. Zwart et al.·Nov 7, 2008SaveLearn
TeV Gamma-ray Astronomy: The Story So FarA snapshot is presented of the present status of our knowledge of the TeV gamma-ray universe. Emphasis is put on observations made using the imaging atmospheric Cherenkov technique. The capabilities…Trevor C. Weekes·Nov 7, 2008SaveLearn
Shell model half-lives for r-process N=82 nucleiWe have performed shell-model calculations of the half-lives and neutron-branching probabilities of the r-process waiting point nuclei at the magic neutron number N=82. These new calculations use a…J. J. Cuenca-Garcia, G. Martinez-Pinedo, K. Langanke et al.·Nov 7, 2008SaveLearn
The Wouthuysen-Field effect in a clumpy intergalactic mediumWe show that, due to the high optical depth of the intergalactic medium to Lyman-alpha photons before the Epoch of Reionization, the Lyman-alpha scattering rate responsible for the Wouthuysen-Field…Jonathan Higgins, Avery Meiksin·Nov 7, 2008SaveLearn
Quenching of Star FormationIn the last decade we have seen an enormous increase in the size and quality of spectroscopic galaxy surveys, both at low and high redshift. New statistical techniques to analyse large portions of…Vivienne Wild, Tamas Budavari, Jeremy Blaizot et al.·Nov 7, 2008SaveLearn
Near Infrared Spectroscopic Monitoring of EXor variables: First ResultsWe present low resolution (R approximately 250) spectroscopy in the near-IR (0.8 to 2.5um) of the EXor variables. These are the initial results (obtained during the period 2007-2008) from a long term…D. Lorenzetti, V. M. Larionov, T. Giannini et al.·Nov 7, 2008SaveLearn
Improved equations for eccentricity generation in hierarchical triple systemsIn a series of papers, we developed a technique for estimating the inner eccentricity in hierarchical triple systems, with the inner orbit being initially circular. However, for certain combinations…Nikolaos Georgakarakos·Nov 7, 2008SaveLearn
Non-LTE modeling of the near UV band of late-type starsWe investigate the ability of both LTE and Non-LTE models to fit the near UV band absolute flux distribution and individual spectral line profiles of three standard stars for which high quality…C. Ian Short, P. H. Hauschildt·Nov 7, 2008SaveLearn
Particle trajectories and acceleration during 3D fan reconnectionContext. The primary energy release in solar flares is almost certainly due to magnetic reconnection, making this a strong candidate as a mechanism for particle acceleration. While particle…S. Dalla, P. K. Browning·Nov 7, 2008SaveLearn
Input from opacity data in computation of pulsation instabilitySeveral types of variable stars are found along the HR diagram whose pulsations are driven by the κ-mechanism. Given their nature, the precise (T eff-L) domain where these pulsators are…Josefina Montalbán, Andrea Miglio·Nov 7, 2008SaveLearn
Eruption of magnetic flux ropes during flux emergenceAims: We investigate the formation of flux ropes in a flux emergence region and their rise into the outer atmosphere of the Sun. Methods: We perform 3D numerical experiments solving the…V. Archontis, T. Torok·Nov 7, 2008SaveLearn
Renewed activity from the X-ray transient SAXJ 1810.8-2609 with INTEGRALWe report on the results of INTEGRAL observations of the neutron star low mass X-ray binary SAX J1810.8-2609 during its latest active phase in August 2007. The current outburst is the first one since…M. Fiocchi, L. Natalucci, J. Chenevez et al.·Nov 7, 2008SaveLearn
CAIXA: a Catalogue of AGN In the XMM-Newton Archive I. Spectral analysisWe present CAIXA, a Catalogue of AGN In the XMM-Newton Archive. It consists of all the radio-quiet X-ray unobscured (NH<2×1022 cm-2) Active Galactic Nuclei (AGN) observed by…Stefano Bianchi, Matteo Guainazzi, Giorgio Matt et al.·Nov 7, 2008SaveLearn
3D acoustic imaging applied to the Baikal Neutrino TelescopeA hydro-acoustic imaging system was tested in a pilot study on distant localization of elements of the Baikal underwater neutrino telescope. For this innovative approach, based on broad band acoustic…K. G. Kebkal, R. Bannasch, O. G. Kebkal et al.·Nov 7, 2008SaveLearn
Lopsided Spiral GalaxiesThe light distribution in the disks of many galaxies is non-axisymmetric or `lopsided' with a spatial extent much larger along one half of a galaxy than the other, as in M101. Recent near-IR…Chanda J. Jog, Francoise Combes·Nov 7, 2008SaveLearn
Rotational spectrum of deuterated and 15N ethyl cyanides: CH3CHDCN and CH2DCH2CN and of CH3CH2C15NEthyl cyanide is an abundant molecule in hot molecular clouds. Lines from 13C isotopically substituted ethyl cyanide were identified in Orion. To enable the search and the possible detection of other…Laurent Margulès, Roman Motiyenko, Karine Demyk et al.·Nov 7, 2008SaveLearn
The seismology programme of CoRoTWe introduce the main lines and specificities of the CoRoT Seismology Core Programme. The development and consolidation of this programme has been made in the framework of the CoRoT Seismology…E. Michel, A. Baglin, M. Auvergne et al.·Nov 7, 2008SaveLearn
Magnetic Structure of Umbral Dots Observed with Hinode Solar Optical TelescopeHigh resolution and seeing-free spectroscopic observation of a decaying sunspot was done with the Solar Optical Telescope aboard Hinode satellite. The target was NOAA 10944 located in the west side…Hiroko Watanabe, Reizaburo Kitai, Kiyoshi Ichimoto et al.·Nov 7, 2008SaveLearn