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- ARC Centre of Excellence for All-sky AstrophysicsAU524 papers
- Centre National de la Recherche ScientifiqueFR491 papers
- The University of SydneyAU368 papers
- ASTRO-3DAU337 papers
- California Institute of TechnologyUS300 papers
- The University of Western AustraliaAU300 papers
- Mount Stromlo ObservatoryAU297 papers
- Max Planck Institute for AstronomyDE296 papers
- University of CambridgeGB295 papers
- Center for Astrophysics Harvard & SmithsonianUS264 papers
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- International Centre for Radio Astronomy ResearchAU257 papers
59 papers · 2 filters
Asymptotic Giant Branch Stars in the Phoenix Dwarf Galaxy
John Menzies, Michael Feast, Patricia Whitelock +3
JHKs near-infrared photometry of stars in the Phoenix dwarf galaxy is presented and discussed. Combining these data with the optical photometry of Massey et al. allows a rather cle…
Observation of an extended VHE gamma-ray emission from MSH 15-52 with CANGAROO-III
T. Nakamori, H. kubo, T. Yoshida +2
We have observed the supernova remnant MSH 15-52 (G320.4-1.2), which contains the gamma-ray pulsar PSR B1509-58, using the CANGAROO-III imaging atmospheric Cherenkov telescope arra…
Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: IV The Controlling Parameters of the Starburst SED
B. Groves, M. Dopita, R. Sutherland +5
We combine the the stellar spectral synthesis code Starburst99, the nebular modelling code MAPPINGSIII, and a 1-D dynamical evolution model of HII regions around massive clusters o…
The Spectral Energy Distribution of Self-gravitating Interstellar Clouds I. Spheres
Joerg Fischera, Michael A. Dopita
We derive the spectral energy distribution (SED) of dusty, isothermal, self gravitating, stable and spherical clouds externally heated by the ambient interstellar radiation field.…
Testing the nature of S0 galaxies using planetary nebula kinematics in NGC 1023
E. Noordermeer, M. R. Merrifield, L. Coccato +9
We investigate the manner in which lenticular galaxies are formed by studying their stellar kinematics: an S0 formed from a fading spiral galaxy should display similar cold outer d…
Dark-Energy Dynamics Required to Solve the Cosmic Coincidence
Chas A. Egan, Charles H. Lineweaver
Dynamic dark energy (DDE) models are often designed to solve the cosmic coincidence (why, just now, is the dark energy density , the same order of magnitude as the matter d…