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
Detection of H3(+) infrared emission lines in Saturn
TL;DR: Three emission lines of the ν 2 fundamental vibration-rotation band of H 3 + have been detected in the ionosphere of Saturn near and at its poles as discussed by the authors, and the observed emission intensities are consistent with a temperature of ≈800 K and total column density of ≃10×10 11 cm −2.
The 8-13 micron spectrum of the young stellar object WL 16
TL;DR: Spectroscopy of WL 16 in the 8-13micron region reveals a spectrum dominated by the hydrocarbon emission features at 77, 86, 1125, and 127 microns as discussed by the authors.
The discovery of a second field methane brown dwarf from sloan digital sky survey commissioning data
Zlatan Tsvetanov,David A. Golimowski,Wei Zheng,Thomas R. Geballe,S. K. Leggett,Holland C. Ford,Arthur F. Davidsen,Alan Uomoto,Xiaohui Fan,Gillian R. Knapp,Michael A. Strauss,J. Brinkmann,D. Q. Lamb,Heidi Jo Newberg,R. Rechenmacher,Donald P. Schneider,Donald G. York,Robert H. Lupton,Jeffrey R. Pier,James Annis,István Csabai,István Csabai,Robert B. Hindsley,Željko Ivesić,Jeffrey A. Munn,Aniruddha R. Thakar,Patrick Waddell +26 more
TL;DR: SDSS J134646.45-003150.4 (hereafter SDSS 1346-00) as mentioned in this paper was selected because of its very red color and stellar appearance and its spectrum between 0.8 and 2.5 µm is dominated by strong absorption bands of H2O and CH4.
Very High Excitation Lines of H$_{2}$ in the Orion Molecular Cloud Outflow
TL;DR: In the case of the Herbig-Haro object HH 7 up to a few percent of the H$2}$ is at a kinetic temperature of 5,000~K as discussed by the authors.
Infrared absorption lines toward ngc 7538 irs 1: abundances of h2, h3+, and co*
TL;DR: In this paper, high-resolution near-infrared absorption spectroscopy of H2, H3+, and CO toward the young high mass object NGC 7538 IRS 1.