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: characterising the near-infrared CO ejecta between 2003 and 2007
TL;DR: In this article, a radiative transfer model was used to fit a spectrum of CO fundamental absorption features around 4.7um to determine the excitation conditions in the line-forming region of Sakurai's Object.
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Silicate dust in the environment of RS Ophiuchi following the 2006 eruption
A. Evans,Charles E. Woodward,L. A. Helton,J. T. van Loon,Richard K. Barry,M. F. Bode,R. J. Davis,J. J. Drake,S. P. S. Eyres,Thomas R. Geballe,Robert D. Gehrz,T. Kerr,Joachim Krautter,David K. Lynch,J. U. Ness,Tim O'Brien,J. P. Osborne,K. L. Page,R. J. Rudy,Ray W. Russell,G. J. Schwarz,Sumner Starrfield,V. H. Tyne +22 more
- 20 Dec 2007
TL;DR: It is concluded that the silicate dust survives the hard radiation impulse and shock blast wave from the RS Ophiuchi eruption, and the existence of the extant dust may have significant implications for understanding the propagation of shocks through the red giant wind and likely wind geometry.
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The Brightening of Re50N: Accretion Event or Dust Clearing?
Hsin-Fang Chiang,Bo Reipurth,Josh Walawender,Michael S. Connelley,Peter Pessev,Thomas R. Geballe,William M. J. Best,Martin Paegert +7 more
TL;DR: In this article, the luminous Class I protostar HBC 494, embedded in the Orion A cloud, is associated with a pair of reflection nebulae, Re50 and Re50N, which appeared sometime between 1955 and 1979.
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Models of infrared spectra of Sakurai's Object (V4334 Sgr) in 1997
TL;DR: Theoretical spectral energy distributions computed for a grid of hydrogen-deficient and carbon-rich model atmospheres have been compared with the observed infrared spectra of V4334 Sgr (Sakurai's Object) on 1997 April 21 and July 13 as mentioned in this paper.
The submillimetre evolution of V4334 Sgr (Sakurai's Object)
TL;DR: In this article, the results of monitoring of V4334 Sgr (Sakurai's Object) at 450 µm and 850 µm with scuba on the James Clerk Maxwell Telescope were reported.
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