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  1. No Access

    Chapter and Conference Paper

    A Long Overdue Synthesis Image of Centaurus A

    Ilana J. Feain, T. J. Cornwell, R. D. Ekers, R. Norris… in Galaxies in the Local Volume (2008)

  2. No Access

    Chapter and Conference Paper

    PSR J1119–6127 and the X-ray emission from high magnetic field radio pulsars

    The existence of radio pulsars having inferred magnetic fields in the magnetar regime suggests that possible transition objects could be found in the radio pulsar population. The discovery of such an object wo...

    M. E. Gonzalez, V. M. Kaspi, F. Camilo… in Isolated Neutron Stars: From the Surface t… (2007)

  3. No Access

    Chapter and Conference Paper

    SN 1987A at Radio Wavelengths

    SN1987A has an intrinsic radio luminosity some four orders of magnitude less than SN1993J at maximum, largely a reflection of the tenuous wind from the progenitor of SN1987A before explosion. Both remnants hav...

    L. Staveley-Smith, R.N. Manchester, B.M. Gaensler, M.J. Kesteven… in Cosmic Explosions (2005)

  4. No Access

    Chapter and Conference Paper

    Radio Polarimetry in the Sothern Galactic Plane Survey

    M. Haverkorn, B. M. Gaensler, N. M. McClure-Griffths… in How does the Galaxy Work? (2004)

  5. No Access

    Chapter and Conference Paper

    Pulsar Bow Shocks as Probes of Warm Neutral Gas

    Pulsars have mean space velocities ≳500 km s−1. The consequent ram pressure results in tight confinement of the star’s energetic wind, driving a bow shock into the surrounding medium. Pulsar bow shocks have long ...

    B. M. Gaensler, B. Stappers, S. Chatterjee, P. Ghavamian… in How does the Galaxy Work? (2004)

  6. No Access

    Chapter and Conference Paper

    The Structure of Galactic Hydrogen on the Largest Scales

    In the past five years studies of Galactic neutral hydrogen (H i) have undergone a resurgence, led primarily by the International Galactic Plane Survey (IGPS). The IGPS is in the process of imaging the H i throug...

    N. M. McClure-Griffiths, J. M. Dickey, B. M. Gaensler… in How does the Galaxy Work? (2004)

  7. No Access

    Chapter and Conference Paper

    Long-Term Variability of Extragalactic Sources at 843 MHZ

    Time variability is commonly observed in the most compact extragalactic radio sources. Low-frequency variability (LFV)—at frequencies <1 GHz—is thought to arise through two different mechanisms, intrinsic and ext...

    R. W. Hunstead, B. M. Gaensler in Extragalactic Radio Sources (1996)