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Featured researches published by Maurizio Toscano.


The Astrophysical Journal | 1998

Spectra of Southern Pulsars

Maurizio Toscano; M. Bailes; R. N. Manchester; J. S. Sandhu

We compare the spectral properties of the millisecond and slow pulsars detected in the Parkes 70 cm survey. The mean spectral index for the millisecond pulsars (MSPs) is -1.9 ± 0.1, whereas the mean spectral index for the slow pulsars is a surprisingly steep: 1.72 ± 0.04. A Kolmogorov-Smirnov test indicates that there is only a 72% probability that the two distributions differ. As a class, MSPs are therefore only fractionally steeper spectrum objects than slow pulsars, as recent literature would suggest. We then model the expected distribution of MSPs in the Galaxy and find that high-frequency surveys, with sensitivities similar to the current Parkes multibeam survey, are likely to detect MSPs in large numbers. The observed distribution of MSPs will be much less isotropic than that resulting from low-frequency surveys, with 50% of detectable MSPs residing within 11° of the Galactic plane in an all-sky survey.


The Astrophysical Journal | 1999

Parallax of PSR J1744–1134 and the Local Interstellar Medium

Maurizio Toscano; M. C. Britton; R. N. Manchester; M. Bailes; J. S. Sandhu; S. R. Kulkarni; S. Anderson

We present the annual trigonometric parallax of PSR J1744-1134 derived from an analysis of pulse times of arrival. The measured parallax, π = 2.8 ± 0.3 mas, ranks among the most precisely determined distances to any pulsar. The parallax distance of 357 pc is over twice that derived from the dispersion measure using the Taylor & Cordes model for the Galactic electron distribution. The mean electron density in the path to the pulsar, ne = (8.8 ± 0.9) × 10-3 cm-3, is the lowest for any disk pulsar. We have compared the ne for PSR J1744-1134 with those for another 11 nearby pulsars with independent distance estimates. We conclude that there is a striking asymmetry in the distribution of electrons in the local interstellar medium. The electron column densities for pulsars in the third Galactic quadrant are found to be systematically higher than for those in the first. The former correlate with the position of the well-known local H I cavity in quadrant 3. The excess electrons within the cavity may be in the form of H II clouds marking a region of interaction between the local hot bubble and a nearby superbubble.


The Astrophysical Journal | 1998

The Orbital Evolution and Proper Motion of PSR J2051–0827

B. W. Stappers; M. Bailes; R. N. Manchester; J. S. Sandhu; Maurizio Toscano

We have carried out high-precision timing observations of the eclipsing binary PSR J2051-0827 in the 3.3 years since its discovery. The data indicate that the orbital period is decreasing at a rate of b = (-11 ± 1) × 10-12. If secular, this orbital period derivative implies a decay time for the orbit of only 25 Myr, which is much shorter than the expected timescale for the ablation of the companion. We have also measured the proper motion of the pulsar to be 5±3 mas yr -->−1. Assuming the pulsar is at the dispersion-measure distance, this implies a very slow transverse velocity v -->t=(30±20) km s -->−1. This combination of low velocity and short orbital period argues against the formation of the system in the standard manner, and we discuss the implications for its evolutionary history.


Archive | 2018

Theory and Philosophy in Education Research: Methodological Dialogues

John Quay; Jennifer Bernadette Bleazby; Steven A. Stolz; Maurizio Toscano; R. Scott Webster

The issue of methodology is a fundamental concern for all who engage in educational research. Presenting a series of methodological dialogues between emi-nent education researchers including Michael Apple, Gert Biesta, Penny Enslin, John Hattie, Nel Noddings, Michael Peters, Richard Pring and Paul Smeyers, this book explores the ways in which they have chosen and developed research methods to style their investigations and frame their arguments. These dialogues address the specialized and technical aspects of conducting edu-cational research, conceptualize the relationship between methodology and the-ory, and provide in-depth discussion of concerns including falsifiability, openness, interpretation and researcher judgement. Foregrounding the researchers’ first-hand experience and knowledge, this book will provide future and current researchers with a deeper comprehension of the place of theory in education research. An illuminating resource for undergraduate and postgraduate researchers alike, Theory and Philosophy in Education Research confronts the intricate complexities of conducting education research in a highly engaging and accessible way.


Monthly Notices of the Royal Astronomical Society | 1999

Millisecond pulsar velocities

Maurizio Toscano; J. S. Sandhu; M. Bailes; R. N. Manchester; M. C. Britton; S. R. Kulkarni; S. Anderson; B. W. Stappers


Icarus | 2000

Chondrule Fine-Grained Mantle Formation by Hypervelocity Impact of Chondrules with a Dusty Gas

Kurt Liffman; Maurizio Toscano


Monthly Notices of the Royal Astronomical Society | 2001

The nature of the PSR J2051—0827 eclipses

B. W. Stappers; M. Bailes; A. G. Lyne; F. Camilo; R. N. Manchester; J. S. Sandhu; Maurizio Toscano; J. F. Bell


Australian Association for Research in Education (NJ1) | 2012

SCIENCE EDUCATION AND THE WORK OF ART

Maurizio Toscano


Archive | 2018

Locating theory in research: opening a conversation

John Quay; Jennifer Bernadette Bleazby; Steven A. Stolz; Maurizio Toscano; R. Scott Webster


Archive | 2014

SUSTAINABILITY EDUCATION AND THE METAPHYSICS OF YASUNÍ-ITT

Andres Montalvo Suarez; Maurizio Toscano

Collaboration


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M. Bailes

Swinburne University of Technology

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R. N. Manchester

Commonwealth Scientific and Industrial Research Organisation

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J. S. Sandhu

California Institute of Technology

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B. W. Stappers

University of Manchester

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John Quay

University of Melbourne

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M. C. Britton

Swinburne University of Technology

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S. Anderson

California Institute of Technology

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S. R. Kulkarni

California Institute of Technology

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