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
The Origin and Vertical Distribution of Carbon Monoxide in Jupiter
TL;DR: In this article, six clearly-resolved lines of the CO 1-0 vibration-rotation band near 4.7 microns have been observed in Jupiter at a resolution of 0.07/cm.
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CO bands in V4334 Sgr (Sakurai's Object): The $\mathsf{^{12}}$C/$\mathsf{^{13}}$C ratio
Ya. V. Pavlenko,Thomas R. Geballe,A. Evans,Barry Smalley,S. P. S. Eyres,V. H. Tyne,L. A. Yakovina +6 more
TL;DR: In this article, the authors present the results of their analysis of a high resolution (R � 30 000) infrared spectrum of V4334 Sgr around the first overtone CO bands, obtained in 1998 July.
Absorption-Line Survey of H$_3^\textbf{+}$ toward the Galactic Center Sources. III. Extent of Warm and Diffuse Clouds
Miwa Goto,Tomonori Usuda,Thomas R. Geballe,Nick Indriolo,Benjamin J. McCall,Thomas Henning,Takeshi Oka +6 more
TL;DR: A follow-up observation on Geballe and Oka (2010, ApJ, 709, L70) showed that absorbing in the R(2, 2) l line of H2O+ is present in J1747 at velocities of between 60 and +100 km s as discussed by the authors.
Spectral evolution of V838 Monocerotis in the optical and near-infrared in early 2002
M. T. Rushton,Thomas R. Geballe,Alexei V. Filippenko,Ryan Chornock,Weidong Li,Douglas C. Leonard,Ryan J. Foley,A. Evans,Barry Smalley,J. Th. van Loon,S. P. S. Eyres +10 more
TL;DR: In this article, optical and near-infrared spectroscopy, and optical spectropolarimetry, of the peculiar variable V838 Mon during the multiple outburst phase in early 2002 are reported.
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Spectroscopy of Mars from 2.04 to 2.44 micrometers during the 1993 opposition: absolute calibration and atmospheric vs mineralogic origin of narrow absorption features.
TL;DR: In this article, the authors presented moderate-resolution (lambda/delta lambda = 300 to 370) reflectance spectra of Mars from 204 to 244 micrometers that were obtained at UKIRT during the 1993 opposition.
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