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Addendum: The Dwarf Irregular Galaxy Sextans A. II. Recent Star Formation History [Astron. J. 114, 2527 (1997)]*

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Robbie C. Dohm-Palmer1, Evan D. Skillman1, A. Saha2, E. Tolstoy3, Mario Mateo4, J. Gallagher5, J. Hoessel5, C. Chiosi6 and R. J. Dufour7

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Footnote
*  Based on observations with the NASA/ESA Hubble Space Telescope obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.
Dates

Issue 1 (1998 January)

Received 0024 February 18



  1. Addendum: The Dwarf Irregular Galaxy Sextans A. II. Recent Star Formation History [Astron. J. 114, 2527 (1997)]

    Robbie C. Dohm-Palmer et al. 1998 The Astronomical Journal 115 152

  2. The coefficients of thermal conductivity and electrical resistivity for a chromium-copper alloy (`Hidurel 6')

    J E S Venart 1964 Br. J. Appl. Phys. 15 1409

  3. All spacetimes with vanishing curvature invariants

    V Pravda et al 2002 Class. Quantum Grav. 19 6213

  4. Indirect exchange interaction in extremely non-parabolic zero-gap semiconductors

    C Lewiner and G Bastard 1980 J. Phys. C: Solid State Phys. 13 2347

  5. The absence of finite-temperature phase transitions in low-dimensional many-body models: a survey and new results

    Axel Gelfert and Wolfgang Nolting 2001 J. Phys.: Condens. Matter 13 R505

  6. Optical and Near-Infrared Imaging of the IRAS 1 Jy Sample of Ultraluminous Infrared Galaxies. II. The Analysis

    S. Veilleux et al. 2002 ApJS 143 315

  7. Causal continuity in degenerate spacetimes

    A Borde et al 1999 Class. Quantum Grav. 16 3457

  8. Quantum dynamics of parasupersymmetric and shape-invariant coupled systems

    A N F Aleixo and A B Balantekin 2007 J. Phys. A: Math. Theor. 40 8417

  9. Mössbauer study of ε-Fe under an external magnetic field

    Saburo Nasu et al 2002 J. Phys.: Condens. Matter 14 11167

  10. Spinning test particles and clock effect in Schwarzschild spacetime

    Donato Bini et al 2004 Class. Quantum Grav. 21 5427

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