Peter Wood
0000-0001-6434-6543
Australian National University
289 papers found
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Ellipsoidal variability and the difference between sequence D and E red giants
Infrared Spectroscopy of Symbiotic Stars. Viii. Orbits for Three S-Type Systems: Ae Arae, Y Coronae Australis, and Ss 73-147
Evolutionary and pulsation properties of AGB stars .
Pulsation of AGB stars in the Small Magellanic Cloud cluster NGC 419 .
Optically bright post-AGB stars in the LMC:. an extensive sample study
Evidence for Mass Ejection Associated With Long Secondary Periods in Red Giants
Long Secondary Periods in variable red giants
Modulations in Multi-Periodic Blue Variables in the Large Magellanic Cloud
IRS Spectra of Unusual Evolved Objects in the Magellanic Clouds
Mass Loss From Low and Intermediate Mass Stars
Metal-rich carbon stars in the Sagittarius dwarf spheroidal galaxy
New Magellanic Cloud R Coronae Borealis and DY Persei type stars from the EROS-2 database: the connection between RCBs, DYPers, and ordinary carbon stars
Ultra-Low Amplitude Variables in the Large Magellanic Cloud—classical Cepheids, Pop. Ii Cepheids, Rv Tau Stars, and Binary Variables
The KECK APERTURE MASKING EXPERIMENT: SPECTRO-INTERFEROMETRY OF THREE MIRA VARIABLES FROM 1.1 TO 3.8 μm
Dust Formation in a Galaxy with Primitive Abundances
The effect of metallicity on Cepheid magnitudes and the distance to M33
New Results on Long Secondary Periods in Red Giants
Spectropolarimetric Observations of the Sequence-D Red Giant Variables S Lep and Z Eri
Dynamical opacity-sampling models of Mira variables - I. Modelling description and analysis of approximations
Nitrogen production in intermediate-mass stars by hot-bottom burning
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