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Lecturer PhD, Astrophysics, University of Sydney, 2003 |
My primary research area are supernova remnants. A supernova explosion marks the endpoint of a massive star evolution, resulting in an expanding shell, the supernova remnant (SNR), followed by slower moving stellar ejecta. The input of energy and freshly produced heavy elements into the interstellar medium make SNRs, dynamically and chemically, one of the most important objects in galaxies.
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Image credit: Life cycles of stars from NASA's Imagine the Universe . The bottom diagram shows evolution of a normal mass star, like our Sun: the star is burning its fuel slowly, and towards the end of the life goes through a red giant phase, ending its life as a white dwarf, and then brown dwarf. The upper diagram shows the evolution of a massive star: the star is burning its fuel more rapidly, goes through a supernova stage and explodes, creating a supernova remnant shell that dissipates back into interstellar medium. The supernova explosion can also leave behind a compact stellar core, a neutron star or a black hole. |
Current research interests:
The Missing Matter, article in Australasian Science
Monash student helps explain a mystery of the universe, ABC Radio National, The Science show with Robyn Williams
Why is research important, 774 ABC Melbourne, Sundays with Alan Brough
Amelia's summer job: finding part of the universe, The Age
Universe's Not-So-Missing Mass, Science Daily
Monash student finds Universe's missing mass, Monash University press release
Fraser-McKelvie, A., Pimbblet, K. A., and Lazendic, J. S., (2011), An estimate of the electron density in filaments of galaxies at z~0.1 MNARS, 415, 1961; ADS link
Lovchinsky, I.; Slane, P.; Gaensler, B. M.; Hughes, J. P.; Ng, C.-Y.; Lazendic, J. S.; Gelfand, J. D.; Brogan, C. L, (2011), A Chandra Observation of Supernova Remnant G350.1-0.3 and Its Central Compact Object, ApJ, vol. 731, 70; ADS link
Lazendic, J. S.; Wardle, M.; Whiteoak, J. B.; Burton, M. G.; Green, A. J. (2010), Multiwavelength observations of the supernova remnant G349.7+0.2 interacting with a molecular cloud, MNRAS, vol. 409, p. 731; ADS link
Lazendic J. S., Dewey D., Schulz N. S., and Canizares C. R., (2006), The Kinematic and Plasma Properties of X-ray Knots in Casssiopea A from the Chandra HETGS, ApJ, vol. 651, p. 250; ADS link
Lazendic J. S., Slane P. O., (2006), Enhanced abundances in three large-diameter mixed-morphology supernova remnants, ApJ, vol. 647, p. 350; ADS link
Lazendic J. S., Slane P., Gaensler B., Reynolds, S., Plucinsky P., Hughes J. P. (2004), A high-resolution study of nonthermal radio and X-ray emission from SNR G347.3-0.5, ApJ, vol. 602, p. 271; ADS link
Lazendic J. S., Slane P., Gaensler B., Plucinsky P., Hughes J. P., Galloway D. K., Crawford F. (2003), X-ray observations of the compact central object in the supernova remnant G347.3-0.5, ApJ, vol. 593, p. 27L; ADS link
ApJ = The Astrophysical Journal MNRAS = Monthly Notices Royal Astronomical Society
Lecturer, 2012 - current
Margaret Clayton Research Fellow, Monash University, 2008- current
Postdoctoral Research Associate, Massachusetts Institute of Technology, 2004-2005
Research Astrophysicist, Harvard-Smithsonian Centre for Astrophysics, 2001-2004
PhD in Astrophysics, University of Sydney, 1998-2001
BSc Honours (First Class) , UWS Nepean, 1997
Undergraduate studies in Mathematics and Astronomy, Belgrade University, 1990-1996