Astrophysical journal

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  Año 2005, Vol. 631, Número 2

  • MAGNETOROTATIONAL INSTABILITY AROUND A ROTATING BLACK HOLE

    M. Yokosawa

    págs. 1051-1061

    

  • ON THE TEMPERATURE PROFILE OF RADIATIVELY EFFICIENT GEOMETRICALLY THIN DISKS IN BLACK HOLE BINARIES WITH THE ASCA GIS

    K. Makishima, K. Ebisawa, A. Kubota

    págs. 1062-1071

    

  • ANTICORRELATED HARD X-RAY TIME LAG IN GRS 1915+105: EVIDENCE FOR A TRUNCATED ACCRETION DISK

    M. Choudhury

    págs. 1072-1081

    

  • DETAILED SPECTRAL ANALYSIS OF THE 260 ks XMM-NEWTON DATA OF 1E 1207.4-5209 AND SIGNIFICANCE OF A 2.1 keV ABSORPTION FEATURE

    K. Mori, C. J. Hailey, J. C. Chonko

    págs. 1082-1093

    

  • TOWARD A UNIFIED LIGHT-CURVE MODEL FOR MULTIWAVELENGTH OBSERVATIONS OF V1974 CYGNI (NOVA CYGNI 1992)

    I. Hachisu

    págs. 1094-1099

    

  • TOWARD AN EMPIRICAL DETERMINATION OF THE ZZ CETI INSTABILITY STRIP

    P. Bergeron, G. Fontaine, A. Gianninas

    págs. 1100-1112

    

  • FAST METHOD FOR CALCULATING CHROMOSPHERIC Ca II AND Mg II RADIATIVE LOSSES

    W. Rammacher

    págs. 1113-1119

    

  • GU BOOTIS: A NEW 0.6 M DETACHED ECLIPSING BINARY

    M. López-Morales

    págs. 1120-1133

    

  • CIRCUMSTELLAR DUST DISKS IN TAURUS-AURIGA: THE SUBMILLIMETER PERSPECTIVE

    J. P. Williams, S. M. Andrews

    págs. 1134-1160

    

  • WHERE ARE THE M DWARF DISKS OLDER THAN 10 MILLION YEARS?

    P. Plavchan

    págs. 1161-1169

    

  • EXPLORING TERRESTRIAL PLANET FORMATION IN THE TW HYDRAE ASSOCIATION

    P. S. Smith, F. J. Low

    págs. 1170-1179

    

  • FORMATION AND EVOLUTION OF PLANETARY SYSTEMS: UPPER LIMITS TO THE GAS MASS IN HD 105

    D. Hollenbach

    págs. 1180-1190

    

  • COULD THE 47 URSAE MAJORIS PLANETARY SYSTEM BE A SECOND SOLAR SYSTEM? PREDICTING THE EARTH-LIKE PLANETS

    L. Liu, H. Kinoshita, J. Ji

    págs. 1191-1197

    

  • A BAYESIAN ANALYSIS OF EXTRASOLAR PLANET DATA FOR HD 73526

    P. C. Gregory

    págs. 1198-1214

    

  • MEASUREMENT OF SPIN-ORBIT ALIGNMENT IN AN EXTRASOLAR PLANETARY SYSTEM

    J. N. Winn, R. W. Noyes, D. Charbonneau, M. J. Holman

    págs. 1215-1226

    

  • ON THE RELATION BETWEEN RECONNECTED MAGNETIC FLUX AND PARALLEL ELECTRIC FIELDS IN THE SOLAR CORONA

    T. G. Forbes, M. Hesse

    págs. 1227-1238

    

  • MAGNETIC FIELD CONFINEMENT IN THE SOLAR CORONA. II. FIELD-PLASMA INTERACTION

    N. Flyer, B. Fornberg

    págs. 1239-1259

    

  • SIMULATION STUDY OF THE FORMATION MECHANISM OF SIGMOIDAL STRUCTURE IN THE SOLAR CORONA

    K. Kusano

    págs. 1260-1269

    

  • DYNAMICS OF THE SOLAR MAGNETIC NETWORK: TWO-DIMENSIONAL MHD SIMULATIONS

    A. A. van Ballegooijen, S. S. Hasan

    págs. 1270-1280

    

  • WHAT IS THE NEON ABUNDANCE OF THE SUN?

    J. N. Bahcall

    págs. 1281-1285

    

  • INFLUENCE OF RANDOM FLUCTUATIONS IN THE ¿-EFFECT ON MERIDIONAL FLOW AND DIFFERENTIAL ROTATION

    M. Rempel

    págs. 1286-1292