Peter Wood
0000-0001-6434-6543
Australian National University
289 papers found
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Oscillatory convective modes in red giants: a possible explanation of the long secondary periods
Post-AGB Stars in the Magellanic Clouds as Tracers of the s-Process Nucleosynthesis
Optically Visible Post-AGB and Post-RGB Stars in the Magellanic Clouds
Understanding the Sequences of Luminous Pulsating Red Giants
VLTI/AMBER Studies of the Atmospheric Structure and Fundamental Parameters of Red Giant and Supergiant Stars
Testing the Dust Shell Model for Long Secondary Period AGB Stars
Infrared Spectroscopy of Symbiotic Stars. X. Orbits for Three S-Type Systems: V1044 Centauri, Hen 3-1213, and Ss 73-96
Understanding AGB evolution in Galactic bulge stars from high-resolution infrared spectroscopy
The pulsation modes, masses and evolution of luminous red giants
What causes the large extensions of red supergiant atmospheres?
Using broad-band photometry to examine the nature of long secondary periods in red giants
Radial Velocity Curves of Ellipsoidal Red Giant Binaries in the Large Magellanic Cloud
Infrared spectroscopy of asymptotic giant branch stars in the Galactic bulge
On the atmospheric structure and fundamental parameters of red supergiants
Effects of moderate abundance changes on the atmospheric structure and colours of Mira variables
Strange pulsation modes in luminous red giants
The immediate precursors of binary planetary nebulae
Optically bright Post-AGB stars in the Magellanic Clouds
The lead discrepancy in intrinsicallys-process enriched post-AGB stars in the Magellanic Clouds
Optically visible post-AGB/RGB stars and young stellar objects in the Small Magellanic Cloud: candidate selection, spectral energy distributions and spectroscopic examination
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