Astrophysical journal

• 

  Año 2005, Vol. 628, Número 2

  • IMPROVED CONSTRAINTS ON THE NEUTRAL INTERGALACTIC HYDROGEN SURROUNDING QUASARS AT REDSHIFTS z > 6

    J. S. B. Wyithe

    págs. 575-582

    

  • ON THE ABSENCE OF GRAVITATIONAL LENSING OF THE COSMIC MICROWAVE BACKGROUND

    J. P. D. Mittaz, R. Lieu

    págs. 583-593

    

  • SIZE IS EVERYTHING: UNIVERSAL FEATURES OF QUASAR MICROLENSING WITH EXTENDED SOURCES

    P. L. Schechter, M. J. Mortonson

    págs. 594-603

    

  • SPITZER DETECTION OF POLYCYCLIC AROMATIC HYDROCARBON AND SILICATE DUST FEATURES IN THE MID-INFRARED SPECTRA OF z ~ 2 ULTRALUMINOUS INFRARED GALAXIES

    L. Yan, R. Chary, L. Armus, H. Teplitz

    págs. 604-610

    

  • INTERPRETATION OF THE RADIO/X-RAY KNOTS OF AGN JETS WITHIN THE INTERNAL SHOCK MODEL FRAMEWORK

    S. Sahayanathan

    págs. 611-616

    

  • UPPER LIMITS ON THE EXTRAGALACTIC BACKGROUND LIGHT FROM THE VERY HIGH ENERGY GAMMA-RAY SPECTRA OF BLAZARS

    M. Schroedter

    págs. 617-628

    

  • THE CLUSTER-SCALE AGN OUTBURST IN HYDRA A

    P. E. J. Nulsen, B. R. McNamara

    págs. 629-636

    

  • Mg II ABSORPTION SYSTEMS IN SLOAN DIGITAL SKY SURVEY QSO SPECTRA

    D. A. Turnshek, D. B. Nestor

    págs. 637-654

    

  • CHANDRA TEMPERATURE PROFILES FOR A SAMPLE OF NEARBY RELAXED GALAXY CLUSTERS

    A. Vikhlinin, M. Markevitch

    págs. 655-672

    

  • A NOTE ON GRAVITATIONAL BROWNIAN MOTION

    D. Merritt

    págs. 673-677

    

  • THE KINEMATIC SIGNATURE OF FACE-ON PEANUT-SHAPED BULGES

    V. P. Debattista

    págs. 678-694

    

  • THE ARAUCARIA PROJECT: NEAR-INFRARED PHOTOMETRY OF CEPHEID VARIABLES IN THE SCULPTOR GALAXY NGC 300

    G. Pietrzynski, W. Gieren

    págs. 695-703

    

  • SUPERNOVA REMNANTS IN THE MAGELLANIC CLOUDS. V. THE COMPLEX INTERIOR STRUCTURE OF THE N206 SUPERNOVA REMNANT

    R. M. Williams

    págs. 704-720

    

  • FORMATION OF MASSIVE BLACK HOLES IN GLOBULAR CLUSTERS

    N. Kawakatu, M. Umemura

    págs. 721-728

    

  • THE UNUSUAL LUMINOSITY FUNCTION OF THE GLOBULAR CLUSTER M10

    D. L. Pollard, E. L. Sandquist

    págs. 729-737

    

  • OB ASSOCIATIONS, SUPERNOVA-GENERATED SUPERBUBBLES, AND THE SOURCE OF COSMIC RAYS

    R. E. Lingenfelter, J. C. Higdon

    págs. 738-749

    

  • FLUORESCENT MOLECULAR HYDROGEN EMISSION IN IC 63: FUSE, HOPKINS ULTRAVIOLET TELESCOPE, AND ROCKET OBSERVATIONS

    K. France, S. R. McCandliss, B.-G. Andersson

    págs. 750-757

    

  • AN UNUSUAL SYSTEM OF H 1 FILAMENTS NEAR WR 5 AND HD 17603

    B. J. Wallace, L. B. G. Knee, M. Normandeau

    págs. 758-768

    

  • PROBING THE SPATIAL DISTRIBUTION OF THE INTERSTELLAR DUST MEDIUM BY HIGH ANGULAR RESOLUTION X-RAY HALOS OF POINT SOURCES

    S. N. Zhang, J. Xiang

    págs. 769-779

    

  • LINE POLARIZATION OF MOLECULAR LINES AT RADIO FREQUENCIES: THE CASE OF DR 21(OH)

    R. M. Crutcher, P. C. Cortes

    págs. 780-788

    

  • HIGH-RESOLUTION MOLECULAR LINE OBSERVATIONS OF THE ENVIRONMENT OF THE CLASS 0 SOURCE B1-IRS

    I. de Gregorio-Monsalvo

    págs. 789-799

    

  • TESTING THE MASSIVE DISK SCENARIO FOR IRAS 18089-1732

    H. Beuther

    págs. 800-810

    

  • THE HERBIG Ae STAR HD 163296 IN X-RAYS

    D. A. Swartz, A. J. Drake, R. F. Elsner

    págs. 811-816

    

  • PROTOSTELLAR DISKS: FORMATION, FRAGMENTATION, AND THE BROWN DWARF DESERT

    C. D. Matzner

    págs. 817-831

    

  • THE CIRCUMSTELLAR ENVIRONMENT OF T TAURI S AT HIGH SPATIAL AND SPECTRAL RESOLUTION

    A. M. Ghez, G. Duchene

    págs. 832-846

    

  • DISSIPATIVE PHOTOSPHERE MODELS OF GAMMA-RAY BURSTS AND X-RAY FLASHES

    P. Meszaros, M. J. Rees

    págs. 847-852

    

  • A NEW MODEL FOR IRON EMISSION LINES AND REBURSTS IN GAMMA-RAY BURST X-RAY AFTERGLOWS

    W. H. Gao, D. M. Wei

    págs. 853-856

    

  • TIME-DEPENDENT NUMERICAL MODEL FOR THE EMISSION OF RADIATION FROM RELATIVISTIC PLASMA

    A. Pe'er, E. Waxman

    págs. 857-866

    

  • OPTICAL AFTERGLOWS OF SHORT GAMMA-RAY BURSTS AND GRB 040924

    Y. Z. Fan, B. Zhang, S. Kobayashi

    págs. 867-872

    

  • ULTRALUMINOUS X-RAY SOURCES: EVIDENCE FOR VERY EFFICIENT FORMATION OF POPULATION III STARS CONTRIBUTING TO THE COSMIC NEAR-INFRARED BACKGROUND EXCESS?

    H. Mii, T. Totani

    págs. 873-878