J
Joss Bland-Hawthorn
Researcher at University of Sydney
Publications - 1157
Citations - 84957
Joss Bland-Hawthorn is an academic researcher from University of Sydney. The author has contributed to research in topics: Galaxy & Stars. The author has an hindex of 136, co-authored 1114 publications receiving 77593 citations. Previous affiliations of Joss Bland-Hawthorn include Macquarie University & Australian National University.
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Journal ArticleDOI
Exploring the dust content of galactic winds with herschel. i. ngc 4631
Marcio Melendez,Sylvain Veilleux,Crystal L. Martin,Chad Engelbracht,Joss Bland-Hawthorn,Gerald Cecil,Fabian Heitsch,A. McCormick,Thomas Müller,David S. N. Rupke,S. H. Teng +10 more
TL;DR: Melendez et al. as mentioned in this paper presented a detailed analysis of deep far-infrared observations of the nearby edge-on star-forming galaxy NGC 4631 obtained with the Herschel Space Observatory.
Proceedings ArticleDOI
DAzLE: The Dark Ages z (redshift) Lyman-alpha Explorer
Anthony Horton,Ian Parry,Joss Bland-Hawthorn,Sonia Cianci,David A. King,Richard G. McMahon,Steve Medlen +6 more
TL;DR: DAzLE as discussed by the authors is an near infrared narrowband differential imager being built by the Institute of Astronomy, Cambridge, in collaboration with the Anglo-Australian observatory for the detection of redshifted Lyman-alpha emission from star forming galaxies at z>7.
Journal ArticleDOI
Evolution of Galactic Discs: Multiple Patterns, Radial Migration and Disc Outskirts
Ivan Minchev,Benoit Famaey,Benoit Famaey,Alice C. Quillen,P. Di Matteo,Francoise Combes,M. Vlajic,Peter Erwin,Joss Bland-Hawthorn +8 more
TL;DR: In this article, the evolution of galactic disks in N-body Tree-SPH simulations is investigated, and it is shown that disks, initially truncated at three scale-lengths, can triple their radial extent, solely driven by secular evolution.
Journal ArticleDOI
The SAMI Pilot Survey: the fundamental and mass planes in three low-redshift clusters
Nicholas Scott,Lisa Fogarty,Matt S. Owers,Matt S. Owers,Scott M. Croom,Matthew Colless,Roger L. Davies,Sarah Brough,Michael Pracy,Joss Bland-Hawthorn,D. Heath Jones,D. Heath Jones,J. T. Allen,Julia J. Bryant,Julia J. Bryant,Luca Cortese,Michael Goodwin,Andrew W. Green,I. S. Konstantopoulos,Jon Lawrence,Jon Lawrence,Samuel N. Richards,Samuel N. Richards,Rob Sharp +23 more
TL;DR: In this paper, the intrinsic scatter of the Fundamental Plane depends on the way in which the velocity dispersion and effective radius are measured, and it is shown that the resulting Mass Plane has further reduced scatter, consistent with zero intrinsic scatter.
Journal ArticleDOI
The SAMI Galaxy Survey: gravitational potential and surface density drive stellar populations -- I. early-type galaxies.
Tania M. Barone,Francesco D'Eugenio,Matthew Colless,Nicholas Scott,Jesse van de Sande,Joss Bland-Hawthorn,Sarah Brough,Julia J. Bryant,Julia J. Bryant,Luca Cortese,Scott M. Croom,Caroline Foster,Michael Goodwin,Iraklis S. Konstantopoulos,Jon Lawrence,Nuria P. F. Lorente,Anne M. Medling,Anne M. Medling,Matt S. Owers,Matt S. Owers,Samuel N. Richards +20 more
TL;DR: For early-type galaxies, the authors found that the color and stellar metallicity [Z/H] correlate more strongly with gravitational potential than with mass $M$, whereas stellar population age correlates best with surface density $Sigma.