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
Sakurai's Object (V4334 Sgr): evolution of the dust shell from 1999 to 2001
TL;DR: In this paper, the authors present fits to 1-5 μm spectra of the dust shell around Sakurai's Object (V4334 Sgr) obtained over the period 1999 May to 2001 September, using the dusty modelling program.
The ice band in IRAS 09371 + 1212
TL;DR: The structure of the absorption feature is reasonably well modeled by a mixture of amorphous and crystalline H2O ice mantles on silicate grains, but discrepancies remain that could indicate other absorbers also.
The Early Spectrophotometric Evolution of V1186 Scorpii (Nova Scorpii 2004 No. 1)
Greg J. Schwarz,Charles E. Woodward,M. F. Bode,A. Evans,S. P. S. Eyres,Thomas R. Geballe,Robert D. Gehrz,Matthew A. Greenhouse,L. A. Helton,William Liller,James E. Lyke,David K. Lynch,David K. Lynch,Tim O'Brien,R. J. Rudy,R. J. Rudy,Ray W. Russell,Ray W. Russell,S. N. Shore,Sumner Starrfield,Tea Temim,J. W. Truran,J. W. Truran,Catherine C. Venturini,R. M. Wagner,Robert Williams,R. K. Zamanov +26 more
TL;DR: In this paper, optical photometry and optical through mid-infrared spectroscopy of the classical nova V1186 Sco was reported, showing that it had a complex light curve with multiple secondary peaks similar to those seen in PW Vul, but the erratic nature of the light curve makes determination of intrinsic properties based on the decline time (e.g., luminosity) problematic.
Detection of the 12.28 micron rotational line of molecular hydrogen in the Orion molecular cloud
TL;DR: The pure rotational S(2) transition of molecular hydrogen at 12.28 microns has been detected in emission from the region of vibrational-rotational line emission in Orion.
Infrared spectroscopy of Nova Cassiopeiae 1993 ‐‐ III. ISO observations
TL;DR: The fine-structure line has been detected in Nova Cassiopeiae 1993 (V705 Cas) by the Short Wavelength Spectrometer on the Infrared Space Observatory (ISO), and preliminary analysis using CLOUDY suggests that oxygen is overabundant relative to solar by at least 25, and that the abundance of neon is 0.5 x solar at most as mentioned in this paper.