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
Galaxy And Mass Assembly (GAMA) : trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments
Mehmet Alpaslan,Mehmet Alpaslan,Simon P. Driver,Simon P. Driver,Aaron S. G. Robotham,Danail Obreschkow,E. Andrae,Michelle E. Cluver,Lee S. Kelvin,Rebecca A. Lange,Matt S. Owers,Matt S. Owers,Edward N. Taylor,Stephen K. Andrews,Steven P. Bamford,Joss Bland-Hawthorn,Sarah Brough,Michael J. I. Brown,Matthew Colless,Luke J. M. Davies,Elizabeth Eardley,Meiert W. Grootes,Andrew M. Hopkins,Rebecca Kennedy,Jochen Liske,Maritza A. Lara-López,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Jon Loveday,Barry F. Madore,Smriti Mahajan,Martin Meyer,Amanda J. Moffett,Peder Norberg,Samantha J. Penny,Kevin A. Pimbblet,Kevin A. Pimbblet,Cristina C. Popescu,Cristina C. Popescu,Mark Seibert,Richard J. Tuffs +40 more
TL;DR: In this paper, the authors explore trends in galaxy properties with Mpc-scale structures using catalogues of environment and large-scale structure from the Galaxy And Mass Assembly (GAMA) survey.
Journal ArticleDOI
Fossil imprint of a powerful flare at the galactic center along the magellanic stream
TL;DR: The Magellanic Stream is a clumpy gaseous structure free of stars trailing behind the Magellan Clouds, passing over the south Galactic pole (SGP) at a distance of at least 50-100 kpc from the Galactic center.
Journal ArticleDOI
The ionized gas in the CALIFA early-type galaxies I. Mapping two representative cases: NGC 6762 and NGC 5966
C. Kehrig,C. Kehrig,Ana Monreal-Ibero,Polychronis Papaderos,José M. Vílchez,J. M. Gomes,J. Masegosa,Sebastián F. Sánchez,Matthew D. Lehnert,R. Cid Fernandes,R. Cid Fernandes,Joss Bland-Hawthorn,D. J. Bomans,I. Márquez,D. Mast,J. A. L. Aguerri,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,R. A. Marino,Anna Pasquali,I. Pérez,Martin Roth,Patricia Sanchez-Blazquez,Bodo L. Ziegler +23 more
TL;DR: In this article, the authors performed a thorough analysis of the ionized gas in two E/S0 galaxies, NGC 6762 and NGC 5966, aiming to shed light on the nature of their warm ionized ISM.
Journal ArticleDOI
Weighing the local dark matter with RAVE red clump stars
Olivier Bienaymé,Benoit Famaey,Arnaud Siebert,Kenneth C. Freeman,Brad K. Gibson,Brad K. Gibson,G. F. Gilmore,Eva K. Grebel,Joss Bland-Hawthorn,Georges Kordopatis,Ulisse Munari,Julio F. Navarro,Quentin A. Parker,Quentin A. Parker,Warren A. Reid,Warren A. Reid,George M. Seabroke,Alessandro Siviero,Matthias Steinmetz,Fred G. Watson,R. F. G. Wyse,Tomaž Zwitter +21 more
TL;DR: In this article, the vertical force and the total mass density distribution up to 2 kpc away from the Galactic plane were determined by fitting a distribution function depending explicitly on three isolating integrals of the motion in a separable potential locally representing the Galactic one with four free parameters.
Journal ArticleDOI
Chemical gradients in the Milky Way from the RAVE data
Corrado Boeche,A. Siebert,T. Piffl,Andreas Just,Matthias Steinmetz,Sanjib Sharma,G. Kordopatis,G. Gilmore,Cristina Chiappini,M. Williams,Eva K. Grebel,Joss Bland-Hawthorn,Bradley Kenneth Gibson,U. Munari,Alessandro Siviero,Olivier Bienaymé,Julio F. Navarro,Quentin A. Parker,Warren Reid,George M. Seabroke,F. G. Watson,R. F. G. Wyse,Tomaž Zwitter +22 more
TL;DR: In this paper, the authors measured the radial and vertical chemical gradients for the elements Mg, Al, Si, Ti, and Fe in the Galactic disc and the gradient variations as a function of the distance from the Galactic plane (Z).