Thomas R. Geballe
University of Hawaii at Manoa
312 Papers
4.5K Citations
Thomas R. Geballe is an academic researcher from University of Hawaii at Manoa. The author has contributed to research in topics: Stars & Brown dwarf. The author has an hindex of 71, co-authored 301 publications.
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Papers
Infrared emission line studies of the structure and excitation of H II regions
TL;DR: In this article, maps of five H II regions in one or more of the infrared fine-structure lines of Ne II (12.8 microns), Ar III (9.0 microns, and S IV (10.5 microns) have been obtained with angular resolutions ranging from 4 to 7 arcsec.
PALOMAR/TRIPLESPEC OBSERVATIONS OF SPITZER/MIPSGAL 24 μm CIRCUMSTELLAR SHELLS: UNVEILING THE NATURES OF THEIR CENTRAL SOURCES
Nicolas Flagey,Alberto Noriega-Crespo,Alberto Noriega-Crespo,Andreea Petric,Thomas R. Geballe +4 more
TL;DR: In this article, near-IR spectroscopic observations of the central sources in 17 circumstellar shells from a sample of more than 400 "bubbles" discovered in the Spitzer/MIPSGAL 24 μm survey of the Galactic plane and in the Cygnus-X region were presented.
Post-equinoctial observations of the ionosphere of Uranus
Henrik Melin,Tom Stallard,Steve Miller,Thomas R. Geballe,Laurence M. Trafton,James O'Donoghue +5 more
TL;DR: Melin et al. as discussed by the authors analyzed ground-based infrared observations of H 3 + emission from the upper atmosphere of Uranus using Gemini North/GNIRS, NASA IRTF/SpeX and VLT/CRIRES.
Water Ice on Triton
Dale P. Cruikshank,Bernard Schmitt,Ted L. Roush,Tobias Owen,Eric Quirico,Thomas R. Geballe,Catherine de Bergh,Mary Jane Bartholomew,Cristina M. Dalle Ore,Cristina M. Dalle Ore,Sylvain Douté,Roland Meier +11 more
TL;DR: In this article, the authors reported the spectroscopic detection of H2O ice on Triton, evidenced by the broad absorptions in the near infrared at 1.87-2.04 micron.
A study of the 3.3 and 3.4 μm emission features in proto-planetary nebulae
TL;DR: In this article, the 3.3 and 3.4 μm emission features of seven carbon-rich proto-planetary nebulae (PPNs) and one young planetary nebula from 3.2 to 3.8 μm were identified.