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researcher

T. Geballe

4 papers hereh-index 7319.9k citations676 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.GA1
same name
  • T. Geballe — 10 papers, h 4
  • T. Geballe — 1 paper, h 10

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.SR2025

Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It will be the Brightest Classical or Recurrent Nova Ever Observed in X-rays

S. Starrfield, M. Bose, C. E. Woodward +11

T Coronae Borealis (TCrB) is a recurrent nova (RN) with recorded outbursts in 1866, and 1946 and possible outbursts in 1217 and 1787. It is predicted to explode again in 2025 or 20…

astro-ph.SR2024

Near-infrared spectroscopy of the LMC recurrent nova LMCN 1968-12a

A. Evans, D. P. K. Banerjee, T. R. Geballe +5

We have obtained near-infrared (0.80−2.45I^¼m) spectra of the recurrent nova LMCN 1968-12a on two occasions during its 2024 August eruption. This is the first near-infrared spectr…

astro-ph.GA2024

Diffuse interstellar bands in the near-infrared: Expanding the reddening range

R. Castellanos, F. Najarro, M. Garcia +2

We have investigated the behaviour of three strong near-infrared diffuse interstellar bands (DIBs) at λ13177 à , λ14680 à , and λ15272 à , on a larger sample of sightlines and o…

astro-ph.SR2024

Haro 5-2: A New Pre-Main Sequence Quadruple Stellar System

Bo Reipurth, C. Briceno, T. R. Geballe +9

We have discovered that the Halpha emission line star Haro 5-2, located in the 3-6 Myr old Ori OB1b association, is a young quadruple system. The system has a 2+2 configuration wit…

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