On binary pulsars and the force of gravityThe energy-momentum budget of the astrophysical systems can be studied by the exact local conservation equation derived by Landau and Lifshitz. We show that a similar equation is valid for the…Davor Palle·May 19, 2026SaveLearn
Tidal torques. A critical review of some techniquesWe point out that the MacDonald formula for body-tide torques is valid only in the zeroth order of e/Q, while its time-average is valid in the first order. So the formula cannot be used for analysis…Michael Efroimsky, James G. Williams·Aug 26, 2012SaveLearn
Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle RecombinationWe investigate the effects of neutrino heating and alpha-particle recombination on the hydrodynamics of core-collapse supernovae. Our focus is on the non-linear dynamics of the shock wave that forms…Rodrigo Fernández, Christopher Thompson·Dec 30, 2008SaveLearn
Asymptotically FRW black holesApplication of concepts like black hole and event horizon in cosmological context are not trivial, as has been shown in the last decade. We introduce special solutions of the LTB family representing…J. T. Firouzjaee, Reza Mansouri·Dec 30, 2008SaveLearn
Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole MergerThe association of an electromagnetic signal with the merger of a pair of supermassive black holes would have many important implications. For example, it would provide new information about gas and…Sean M. O'Neill, M. Coleman Miller, Tamara Bogdanovic et al.·Dec 30, 2008SaveLearn
A Gamma-Ray Burst/Pulsar for Cosmic-Ray Positrons with a Dark Matter-like SpectrumWe propose that a nearby gamma-ray burst (GRB) or GRB-like (old, single and short-lived) pulsar/supernova remnant/microquasar about 105-6 years ago may be responsible for the excesses of…Kunihito Ioka·Dec 30, 2008SaveLearn
Catastrophic Photo-z Errors and the Dark Energy Parameter Estimates with Cosmic ShearWe study the impact of catastrophic errors occurring in the photometric redshifts of galaxies on cosmological parameter estimates with cosmic shear tomography. We consider a fiducial survey with…L. Sun, Z. -H. Fan, C. Tao et al.·Dec 30, 2008SaveLearn
Ultraviolet Spectra of Local Galaxies and their Link with the High-z PopulationThe new generation of 8 to 10m class telescope is providing us with high-quality spectral information on the rest-frame ultraviolet region of star-forming galaxies at cosmological distances. The data…Claus Leitherer·Dec 30, 2008SaveLearn
Biases and Uncertainties in Physical Parameter Estimates of Lyman Break Galaxies from Broad-band PhotometryWe investigate the biases and uncertainties in estimates of physical parameters of high-redshift Lyman break galaxies (LBGs), such as stellar mass, mean stellar population age, and star formation…Seong-Kook Lee, Rafal Idzi, Henry C. Ferguson et al.·Dec 30, 2008SaveLearn
Stellar Ages from Stellar RotationOur ability to determine stellar ages from measurements of stellar rotation, hinges on how well we can measure the dependence of rotation on age for stars of different masses. Rotation periods for…Soren Meibom·Dec 30, 2008SaveLearn
An Evolutionary Considerations for V228 from 47 TucWe perform evolutionary calculations of binary stars to find progenitors of system with parameters similar to the eclipsing binary system V228. We show that a V228 binary system may be formed…Marek J. Sarna·Dec 30, 2008SaveLearn
Source region of the 2003 November 18 CME that led to the strongest magnetic storm of cycle 23The super-storm of November 20, 2003 was associated with a high speed coronal mass ejection which originated in the NOAA AR 10501 on November 18. This coronal mass ejection had severe terrestrial…N. Srivastava, S. Mathew, R. Louis et al.·Dec 30, 2008SaveLearn
Further progress on solar age calibrationWe recalibrate a standard solar model seismologically to estimate the main-sequence age of the Sun. Our procedure differs from what we have done in the past by removing from the observed frequencies…Günter Houdek, Douglas Gough·Dec 30, 2008SaveLearn
Bulk viscosity of strange matter and r-modes in neutron starsWe discuss bulk viscosity due to non-leptonic processes involving hyperons and Bose-Einstein condensate of negatively charged kaons in neutron stars. It is noted that the hyperon bulk viscosity…Debarati Chatterjee, Debades Bandyopadhyay·Dec 30, 2008SaveLearn
Necessity of Dark Matter in Modified Newtonian Dynamics within Galactic Scales? - Testing the Covariant MOND in Elliptical LensesModified Newtonian Dynamics (MOND) and its relativistic version - TeVeS offer us an alternative perspective to understand the universe without the demand of the elusive cold dark matter. This MONDian…M. C. Chiu, Y. Tian, C. M. Ko·Dec 30, 2008SaveLearn
Origin of Europa and the Galilean SatellitesEuropa is believed to have formed near the very end of Jupiter's own accretion, within a circumplanetary disk of gas and solid particles. We review the formation of the Galilean satellites in the…Robin M. Canup, William R. Ward·Dec 30, 2008SaveLearn
Correlated variability in the blazar 3C 454.3The blazar 3C 454.3 was revealed by the Fermi Gamma-ray Space Telescope to be in an exceptionally high flux state in July 2008. Accordingly, we performed a multi-wavelength monitoring campaign on…E. W. Bonning, C. Bailyn, C. M. Urry et al.·Dec 30, 2008SaveLearn
Compressed sensing imaging techniques for radio interferometryRadio interferometry probes astrophysical signals through incomplete and noisy Fourier measurements. The theory of compressed sensing demonstrates that such measurements may actually suffice for…Y. Wiaux, L. Jacques, G. Puy et al.·Dec 29, 2008SaveLearn
Detecting Solar Neutrino Flare in Megaton and km3 detectorsTo foresee a solar flare neutrino signal we infer its upper and lower bound. The upper bound was derived since a few years by general energy equipartition arguments on observed solar particle flare.…Daniele Fargion, Paola Di Giacomo·Dec 29, 2008SaveLearn
Untwisting magnetospheres of neutron starsMagnetospheres of neutron stars are anchored in the rigid crust and can be twisted by sudden crustal motions ("starquakes"). The twisted magnetosphere does not remain static and gradually…Andrei M. Beloborodov·Dec 29, 2008SaveLearn
High Accuracy Near-infrared Imaging Polarimetry with NICMOSThe findings of a nine orbit calibration plan carried out during HST Cycle 15, to fully determine the NICMOS camera 2 (2.0 micron) polarization calibration to high accuracy, are reported. Recently…D. Batcheldor, G. Schneider, D. C. Hines et al.·Dec 29, 2008SaveLearn
Active Galactic Nuclei, Radio Jets and Acceleration of UHECRsWe present the general properties of the Active Galactic Nuclei (AGNs) and discuss the origin and structure of jets that are associated to a fraction of these objects. We then we address the problems…S. Massaglia·Dec 29, 2008SaveLearn
Measuring interstellar magnetic fields by radio synchrotron emissionRadio synchrotron emission, its polarization and its Faraday rotation are powerful tools to study the strength and structure of interstellar magnetic fields. The total intensity traces the strength…Rainer Beck·Dec 29, 2008SaveLearn
The CHilean Automatic Supernova sEarch (CHASE)The CHASE project started in 2007 with the aim of providing young southern supernovae (SNe) to the Carnegie Supernova Project (CSP) and Millennium Center for Supernova Studies (MCSS) follow-up…G. Pignata, J. Maza, M. Hamuy et al.·Dec 29, 2008SaveLearn
Friedmann cosmology with bulk viscosity: a concrete model for dark energyThe universe content is considered as a non-perfect fluid with bulk viscosity and can be described by a general equation of state (endowed some deviation from the conventionally assumed cosmic…X H Meng, X Dou·Dec 29, 2008SaveLearn