Explosive Nucleosynthesis of Weak r-Process Elements in Extremely Metal-Poor Core-Collapse SupernovaeThere have been attempts to fit the abundance patterns of extremely metal-poor stars with supernova nucleosynthesis models for the lighter elements than Zn. On the other hand, observations have…N. Izutani, H. Umeda, N. Tominaga·Oct 31, 2008SaveLearn
Regularities in the frequency spacings of Delta Scuti stars and the s-f DiagramStatistical analyses of several Delta Scuti stars (FG Vir, 44 Tau, BL Cam and others) show that the photometrically observed frequencies cluster around the frequencies of the radial modes over many…M. Breger, P. Lenz, A. A. Pamyatnykh·Oct 31, 2008SaveLearn
Radiation processes around accreting black holesAccreting sources such as AGN, X-ray binaries or gamma-ray bursts are known to be strong, high energy emitters. The hard emission is though to originate from plasmas of thermal and/or non-thermal…R. Belmont, J. Malzac, A. Marcowith·Oct 31, 2008SaveLearn
Simulating acceleration and radiation processes in X-ray binariesThe high energy emission of microquasars is thought to originate from high energy particles. Depending on the spectral state, the distribution of these particles can be thermal with a high…R. Belmont, J. Malzac, A. Marcowith·Oct 31, 2008SaveLearn
Chemical Diversity in High-Mass Star FormationMassive star formation exhibits an extremely rich chemistry. However, not much evolutionary details are known yet, especially at high spatial resolution. Therefore, we synthesize previously published…H. Beuther, Q. Zhang, E. A. Bergin et al.·Oct 31, 2008SaveLearn
Suzaku observations of metallicity distribution in the intracluster medium of the NGC 5044 groupThe metallicity distribution in the intracluster medium of the NGC 5044 group was studied up to 0.3 r180 using the XIS instrument on board the Suzaku satellite. Abundances of O, Mg, Si, S, and Fe…Madoka Komiyama, Kosuke Sato, Ryo Nagino et al.·Oct 31, 2008SaveLearn
Galaxy Interactions, Star Formation History, and Bulgeless GalaxiesHierarchical Lambda CDM models provide a successful paradigm for the growth of dark matter on large scales, but they face important challenges in predicting how the baryonic components of galaxies…Shardha Jogee·Oct 31, 2008SaveLearn
Intergalactic dust and its photoelectric heatingWe have examined the dust photoelectric heating in the intergalactic medium (IGM). The heating rate in a typical radiation field of the IGM is represented by Γ pe = 1.2×10-34 erg…Akio K. Inoue, Hideyuki Kamaya·Oct 31, 2008SaveLearn
Science with UT's Dichroic-Mirror Camera (DMC), 15-band simultaneous imagerWe introduce the Dichroic-Mirror Camera (DMC), an instrument developed at the University of Tokyo which is capable of performing simultaneous imaging in fifteen bands. The main feature of the DMC is…Hanindyo Kuncarayakti, Mamoru Doi, Hakim L. Malasan et al.·Oct 31, 2008SaveLearn
Dynamics of Galactic Disks and Mergers at z~1.6: Spatially Resolved Spectroscopy with Keck Laser Guide Star Adaptive OpticsWe present 0.2" resolution near-infrared integral field spectroscopy of H-alpha emission from six star forming galaxies at z~1.6 (look-back time of ~9.6 Gyr). These observations were obtained…Shelley A. Wright, James E. Larkin, David R. Law et al.·Oct 31, 2008SaveLearn
Cosmic transparency: A test with the baryon acoustic feature and type Ia supernovaeConservation of the phase-space density of photons plus Lorentz invariance requires that the cosmological luminosity distance be larger than the angular diameter distance by a factor of (1+z)2,…Surhud More, Jo Bovy, David W. Hogg·Oct 30, 2008SaveLearn
Jet-BLR connection in the radio galaxy 3C 390.3Variations of the optical continuum emission in the radio galaxy 3C 390.3 are compared to the properties of radio emission from the compact, sub-parsec-scale jet in this object. We showed that very…T. G. Arshakian, J. Leon-Tavares, A. P. Lobanov et al.·Oct 30, 2008SaveLearn
Linear dynamics of weakly viscous accretion disks: A disk analog of Tollmien-Schlichting wavesThis paper discusses new perspectives and approaches to the problem of disk dynamics where, in this study, we focus on the effects of viscous instabilities influenced by boundary effects. The…O. M. Umurhan, G. Shaviv·Oct 30, 2008SaveLearn
Discovery of molecular shells associated with supernova remnants. (II) Kesteven 75The young composite supernova remnant (SNR) Kesteven 75, with a pulsar wind nebula at its center, has an unusual morphology with a bright southern half-shell structure in multiwavelengths. The…Yang Su, Yang Chen, Ji Yang et al.·Oct 30, 2008SaveLearn
Solar system tests do not rule out 1/R gravityWe argue that Solar system tests do not rule out 1/R gravity at least due to the reason addressed in Phys. Rev. D 74 (2006) 121501 [astro-ph/0610483] (ref. [1]) and subsequent published papers. Ref.…Qasem Exirifard·Oct 30, 2008SaveLearn
Cosmological Perturbations in Models of Coupled Dark EnergyModels in which dark energy interacts with dark matter have been proposed in the literature to help explain why dark energy should only come to dominate in recent times. In this paper, we present a…Sirichai Chongchitnan·Oct 30, 2008SaveLearn
The PAMELA Positron Excess from Annihilations into a Light BosonRecently published results from the PAMELA experiment have shown conclusive evidence for an excess of positrons at high (~ 10 - 100 GeV) energies, confirming earlier indications from HEAT and AMS-01.…Ilias Cholis, Douglas P. Finkbeiner, Lisa Goodenough et al.·Oct 30, 2008SaveLearn
Resolution of the Distance Ambiguity for Galactic HII RegionsWe resolve the kinematic distance ambiguity for 266 inner Galaxy HII regions out of a sample of 291 using existing HI and 13CO sky surveys. Our sample contains all HII regions with measured radio…L. D. Anderson, T. M. Bania·Oct 30, 2008SaveLearn
A High Precision, Optical Polarimeter to Measure Inclinations of High Mass X-Ray BinariesWe present commissioning data for the POLISH instrument obtained on the Hale 5-m telescope. The goal of this high precision polarimeter is to constrain orbital inclination of high mass X-ray binaries…Sloane J. Wiktorowicz, Keith Matthews·Oct 30, 2008SaveLearn
Impacts of WIMP dark matter upon stellar evolution: main-sequence starsThe presence of large amounts of WIMP dark matter in stellar cores has been shown to have significant effects upon models of stellar evolution. We present a series of detailed grids of…Pat Scott, Malcolm Fairbairn, Joakim Edsjö·Oct 30, 2008SaveLearn
A spectroscopic survey of dwarf galaxies in the Coma Cluster: Stellar populations, environment and downsizingWe investigate the stellar populations in a sample of 89 faint (M*+2 to M*+4) red galaxies in the Coma cluster, using high S/N spectroscopy from the MMT. Our sample is drawn from two 1-degree fields,…Russell J. Smith, John R. Lucey, Michael J. Hudson et al.·Oct 30, 2008SaveLearn
Fluorescent excitation of Balmer lines in gaseous nebulae: case D(abridged) Non-ionizing stellar continua are a source of photons for continuum pumping in the hydrogen Lyman transitions. In the environments where these transitions are optically thick, deexcitation…V. Luridiana, S. Simon-Diaz, M. Cervino et al.·Oct 30, 2008SaveLearn
TeV variability in blazars: how fast can it be?Recent Cerenkov observations of the two BL Lac objects PKS 2155-304 and Mkn 501 revealed TeV flux variability by a factor ~2 in just 3-5 minutes. Even accounting for the effects of relativistic…G. Ghisellini, F. Tavecchio, G. Bodo et al.·Oct 30, 2008SaveLearn
LISA detection of massive black hole binaries: imprint of seed populations and of exterme recoilsAll the physical processes involved in the formation, merging, and accretion history of massive black holes along the hierarchical build--up of cosmic structures are likely to leave an imprint on the…A. Sesana, M. Volonteri, F. Haardt·Oct 30, 2008SaveLearn
Distance determination to 12 Type II Supernovae using the Expanding Photosphere MethodWe used early time photometry and spectroscopy of 12 Type II plateau Supernovae (SNe IIP) to derive their distances using the Expanding Photosphere Method (EPM). We performed this study using two…Matias I. Jones·Oct 30, 2008SaveLearn