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researcher

G. Shaw

3 papers hereh-index 211 citations4 works total

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

author position
  • middle author1
  • last author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.SR1
same name
  • G. Shaw — 1 paper, h 1
  • G. Shaw — 1 paper, h 17
  • G. Shaw — 1 paper, h 1

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

3 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.HE2025

Revealing Physical Properties of a Tidal Disruption Event: iPTF16fnl

Mageshwaran Tamilan, Gargi Shaw, Sudip Bhattacharyya +1

Tidal disruption event (TDE) iPTF16fnl shows a relatively low optical flare with observationally very weak X-ray emission and the spectroscopic property that the helium emission li…

astro-ph.HE2024

XMM-Newton high-resolution spectroscopy of EXO 0748-676 after its re-emergence from a long quiescence

Sayantan Bhattacharya, Sudip Bhattacharyya, Gargi Shaw

EXO 0748-676 is a well-studied, high-inclination, dipping, and eclipsing neutron star low-mass X-ray binary that has recently emerged from 16 years of quiescence into a new outburs…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.