Astrophysical journal

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  Año 2003, Vol. 596, Número 1

  • PROBING BEYOND THE EPOCH OF HYDROGEN REIONIZATION WITH 21 CENTIMETER RADIATION

    B. Ciardi, P. Madau

    págs. 1-8

    

  • THE THERMAL MEMORY OF REIONIZATION HISTORY

    L. Hui, Z. Haiman

    págs. 9-18

    

  • CONSTRAINED SIMULATIONS OF THE REAL UNIVERSE: THE LOCAL SUPERCLUSTER

    Y. Hoffman, A. Klypin, A. V. Kravtsov

    págs. 19-33

    

  • FORMATION OF THE FIRST SUPERMASSIVE BLACK HOLES

    V. Bromm, A. Loeb

    págs. 34-46

    

  • GALAXY FORMATION: COLD DARK MATTER, FEEDBACK, AND THE HUBBLE SEQUENCE

    J. Sommer-Larsen

    págs. 47-66

    

  • DISCOVERY OF A CLUSTERED QUASAR PAIR AT z &unknown; 5: BIASED PEAKS IN EARLY STRUCTURE FORMATION

    S. G. Djorgovski

    págs. 67-71

    

  • A RELATION BETWEEN SUPERMASSIVE BLACK HOLE MASS AND QUASAR METALLICITY?

    M. Dietrich, F. Hamann, C. Warner

    págs. 72-84

    

  • Fe XXV AND Fe XXVI DIAGNOSTICS OF THE BLACK HOLE AND ACCRETION DISK IN ACTIVE GALAXIES: CHANDRA TIME-RESOLVED GRATING SPECTROSCOPY OF NGC 7314

    T. Yaqoob, I. M. George, T. R. Kallman, U. Padmanabhan

    págs. 85-104

    

  • EXTENDED X-RAY EMISSION AROUND 4C 41.17 AT z = 3.8

    I. Smail, Robert J. Ivison, C. Scharf

    págs. 105-113

    

  • CAN A DUSTY WARM ABSORBER MODEL REPRODUCE THE SOFT X-RAY SPECTRA OF MCG -6-30-15 AND MARKARIAN 766?

    S. M. Kahn, G. Branduardi-Raymont, M. Sako

    págs. 114-128

    

  • EVOLUTION OF CLUSTER ELLIPTICAL GALAXIES

    L. F. Barrientos

    págs. 129-142

    

  • THE STAR-FORMING DWARF GALAXY POPULATIONS OF TWO z ~ 0.4 CLUSTERS: MS 1512.4+3647 AND A851

    C. L. Martin, J. M. Lotz, H. C. Ferguson

    págs. 143-158

    

  • CIRCULATION FLOWS: COOLING FLOWS WITH BUBBLE RETURN

    W. G. Mathews, F. Brighenti

    págs. 159-169

    

  • SPATIAL DISTRIBUTIONS OF A3558 IN THE CORE REGION OF THE SHAPLEY SUPERCLUSTER

    A. Furuzawa, K. Kondou, F. Akimoto

    págs. 170-180

    

  • CHANDRA OBSERVATION OF THE CORE OF THE GALAXY CLUSTER AWM 7

    T. Furusho, N. Y. Yamasaki

    págs. 181-189

    

  • A CHANDRA STUDY OF THE COMPLEX STRUCTURE IN THE CORE OF 2A 0335+096

    P. Mazzotta, A. C. Edge, M. Markevitch

    págs. 190-203

    

  • CONSTRAINTS OF THE CLUMPINESS OF DARK MATTER HALOS THROUGH HEATING OF THE DISK GALAXIES

    E. Ardi, T. Tsuchiya

    págs. 204-215

    

  • CONSTRAINTS ON COLD DARK MATTER IN THE GAMMA-RAY HALO OF NGC 253

    S. Yanagita, R. Enomoto, T. Yoshida

    págs. 216-219

    

  • BRANCH, SPUR, AND FEATHER FORMATION IN SPIRAL GALAXIES

    S. Chakrabarti

    págs. 220-239

    

  • KINEMATIC MASSES OF SUPER-STAR CLUSTERS IN M82 FROM HIGH-RESOLUTION NEAR-INFRARED SPECTROSCOPY

    A. M. Gilbert, N. McCrady

    págs. 240-252

    

  • DEEP HUBBLE SPACE TELESCOPE IMAGING OF IC 1613. II. THE STAR FORMATION HISTORY

    E. D. Skillman

    págs. 253-272

    

  • THE SPECTRUM OF INTEGRATED MILLIMETER FLUX OF THE MAGELLANIC CLOUDS AND 30 DORADUS FROM TOPHAT AND DIRBE DATA

    J. E. Aguirre, J. J. Bezaire

    págs. 273-286

    

  • SUPERNOVA REMNANT CANDIDATES IN THE 30 DORADUS NEBULA

    J. S. Lazendic

    págs. 287-298

    

  • RR LYRAE STARS IN GALACTIC GLOBULAR CLUSTERS. II. A THEORETICAL APPROACH TO VARIABLES IN M3

    M. Marconi, M. Di Criscienzo, F. Caputo

    págs. 299-313

    

  • THE FATE OF STAR CLUSTERS NEAR THE GALACTIC CENTER. I. ANALYTIC CONSIDERATIONS

    S. L. W. McMillan

    págs. 314-322

    

  • X-RAY EMISSION FROM A SAMPLE OF YOUNG SUPERNOVAE

    J. N. Bregman

    págs. 323-327

    

  • Interstellar hydroxyl masers in the Galaxy. II. Zeeman pairs and the galactic magnetic field.

    M. J. Reid, Karl M. Menten, V. L. Fish, A. L. Argon

    págs. 328-343

    

  • DUAL COMETARY H II REGIONS IN DR 21: BOW SHOCKS OR CHAMPAGNE FLOWS?

    C. J. Cyganowski

    págs. 344-349

    

  • ABUNDANCES AND PHYSICAL CONDITIONS IN THE INTERSTELLAR GAS TOWARD HD 185418

    P. Sonnentrucker

    págs. 350-361

    

  • MOLECULAR COUNTERPARTS OF ULTRACOMPACT H II REGIONS WITH EXTENDED ENVELOPES

    K.-T. Kim, B.-C. Koo

    págs. 362-382