Accretion Properties of A Sample of Hard X-ray (<60keV) Selected Seyfert 1 GalaxiesWe examine the accretion properties in a sample of 42 hard (3-60keV) X-ray selected nearby broad-line AGNs. The energy range in the sample is harder than that usually used in the similar previous…J. Wang, Y. F. Mao, J. Y. Wei·Nov 20, 2008SaveLearn
Analytic Expressions for the Surface Brightness Profile of GRB Afterglow ImagesThe exact profile of a gamma-ray burst (GRB) afterglow image on the plane of the sky can provide important constraints on the underlying physics. In particular, it can test whether the magnetic field…Jonathan Granot·Nov 20, 2008SaveLearn
Alignment of galaxy spins in the vicinity of voidsWe provide limits on the alignment of galaxy orientations with the direction to the void center for galaxies lying near the edges of voids. We locate spherical voids in volume limited samples of…Anže Slosar, Martin White·Nov 19, 2008SaveLearn
No evidence for mass segregation in massive young clustersAims. We investigate the validity of the mass segregation indicators commonly used in analysing young stellar clusters. Methods. We simulate observations by constructing synthetic seeing-limited…J. Ascenso, J. Alves, M. T. V. T. Lago·Nov 19, 2008SaveLearn
Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic NucleiWe present hydrodynamical N-body simulations of clusters of galaxies with feedback taken from semi-analytic models of galaxy formation. The advantage of this technique is that the source of feedback…C. J. Short, P. A. Thomas·Nov 19, 2008SaveLearn
VLBI Observations of SN 2008DWe report on two epochs of very-long-baseline interferometry (VLBI) observations of the Type Ib/c supernova SN 2008D, which was associated with the X-ray outburst XRF 080109. At our first epoch, at t…M. F. Bietenholz, A. M. Soderberg, N. Bartel·Nov 19, 2008SaveLearn
Black hole quasinormal mode spectroscopy with LISAThe signal-to-noise ratio (SNR) for black hole quasinormal mode sources of low-frequency gravitational waves is estimated using a Monte Carlo approach that replaces the all-sky average approximation.…Manish M. Jadhav, Lior M. Burko·Nov 19, 2008SaveLearn
Mean-field dynamos in random Arnold-Beltrami-Childress and Roberts flowsWe study magnetic field evolution in flows with fluctuating in time governing parameters in electrically conducting fluid. We use a standard mean-field approach to derive equations for large-scale…N. Kleeorin, I. Rogachevskii, D. Sokoloff et al.·Nov 19, 2008SaveLearn
Quantifying the fast outflow in the luminous Seyfert galaxy PG1211+143We report two new XMM-Newton observations of PG1211+143 in December 2007, again finding evidence of the fast outflow of highly ionised gas first detected in 2001. Stacking the new spectra with those…K. A. Pounds, J. N. Reeves·Nov 19, 2008SaveLearn
An extensive photometric study of the Blazhko RR Lyrae star MW Lyr: II. Changes in the physical parametersThe analysis of the multicolour photometric observations of MW Lyr, a large modulation amplitude Blazhko variable, shows for the first time how the mean global physical parameters vary during the…J. Jurcsik, Á. Sódor, B. Szeidl et al.·Nov 19, 2008SaveLearn
Expected high energy emission from GRB 080319B and origins of the GeV emission of GRBs 080514B, 080916C and 081024BWe calculate the high energy (sub-GeV to TeV) prompt and afterglow emission of GRB 080319B that was distinguished by a naked-eye optical flash and by an unusual strong early X-ray afterglow. There…Yuan-Chuan Zou, Yi-Zhong Fan, Tsvi Piran·Nov 19, 2008SaveLearn
New SETI Sky Surveys for Radio PulsesBerkeley conducts 7 SETI programs at IR, visible and radio wavelengths. Here we review two of the newest efforts, Astropulse and Fly's Eye. A variety of possible sources of microsecond to…Andrew Siemion, Joshua Von Korff, Peter McMahon et al.·Nov 19, 2008SaveLearn
The [O II] lambda 3727 Luminosity Function at z ~ 1We measure the evolution of the [OII]lambda 3727 luminosity function at 0.75<z<1.45 using high-resolution spectroscopy of ~14,000 galaxies observed by the DEEP2 galaxy redshift survey. We find that…Guangtun Zhu, John Moustakas, Michael R. Blanton·Nov 19, 2008SaveLearn
On the gravitational content of molecular clouds and their cores(Abridged) The gravitational term for clouds and cores entering in the virial theorem is usually assumed to be equal to the gravitational energy, since the contribution to the gravitational force…Javier Ballesteros-Paredes, Gilberto C. Gómez, Bárbara Pichardo et al.·Nov 19, 2008SaveLearn
Diffuse Extragalactic Background RadiationAttenuation of high--energy gamma rays by pair--production with UV, optical and IR background photons provides a link between the history of galaxy formation and high--energy astrophysics. We present…Joel R. Primack, Rudy C. Gilmore, Rachel S. Somerville·Nov 19, 2008SaveLearn
Comprehensive Observations of a Solar Minimum CME with STEREOWe perform the first kinematic analysis of a CME observed by both imaging and in situ instruments on board STEREO, namely the SECCHI, PLASTIC, and IMPACT experiments. Launched on 2008 February 4, the…B. E. Wood, R. A. Howard, S. P. Plunkett et al.·Nov 19, 2008SaveLearn
Wide Area X-ray Surveys for AGN and Starburst GalaxiesWhile often the point sources in X-ray surveys are dominated by AGN, with the high sensitivity of modern X-ray telescopes such as Chandra and XMM-Newton normal/starburst galaxies are also being…A. Ptak·Nov 19, 2008SaveLearn
The chromospherically active binary star EI Eridani II. Long-term Doppler imagingData from 11 years of continuous spectroscopic observations of the active RS CVn-type binary star EI Eridani - gained at NSO/McMath-Pierce, KPNO/Coude Feed and during the MUSICOS 98 campaign - were…A. Washuettl, K. G. Strassmeier, M. Weber·Nov 19, 2008SaveLearn
Impact of sub-solar metallicities on photometric redshiftsWith the advent of deep photometric surveys the use of photometric redshifts, obtained with a variety of techniques, has become more and more widespread. Giving access to galaxies with a wide range…Ralf Kotulla, Uta Fritze·Nov 19, 2008SaveLearn
Angular momentum and clustering properties of early dark matter halosIn this paper we study the angular momentum properties of simulated dark matter halos at high redshift that likely host the first stars in the Universe. Calculating the spin distributions of these…Andrew J. Davis, Priyamvada Natarajan·Nov 19, 2008SaveLearn
Photometric redshifts for the CFHTLS-WideWe want to derive bias free, accurate photometric redshifts for those fields of the CFHTLS-Wide data which are covered in the u*, g', r', i' and z' filters and are public on January 2008. These are…Fabrice Brimioulle, Michael Lerchster, Stella Seitz et al.·Nov 19, 2008SaveLearn
Hαspectropolarimetry of RY Tau and PX VulAims: To detect line effects using spectropolarimetry in order to find evidence of rotating disks and their respective symmetry axes in T Tauri stars. Methods: We used the IAGPOL imaging polarimeter…A. Pereyra, A. M. Magalhães, F. X. de Araújo·Nov 19, 2008SaveLearn
Star Formation from Spitzer (Lyman) to Spitzer (Space Telescope) and BeyondA summary of JENAM 2008 Symposium 9 "Star Formation from Spitzer (Lyman) to Spitzer (Space Telescope) and Beyond", held in Vienna, 10-12 September 2008.Joao Alves, Virginia Trimble·Nov 19, 2008SaveLearn
The location and kinematics of the coronal-line emitting regions in AGNWe use the photoionisation code Cloudy to determine both the location and the kinematics of the optical forbidden, high ionisation line (hereafter, FHIL) emitting gas in the narrow line Seyfert 1…J. R. Mullaney, M. J. Ward, C. Done et al.·Nov 19, 2008SaveLearn
Kinematic properties of early-type galaxy haloes using planetary nebulaeWe present new planetary nebulae (PNe) positions, radial velocities, and magnitudes for 6 early-type galaxies obtained with the Planetary Nebulae Spectrograph, their two-dimensional velocity and…L. Coccato, O. Gerhard, M. Arnaboldi et al.·Nov 19, 2008SaveLearn