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J. Goldstein

4 papers hereh-index 181.1k citations38 works total

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

author position
  • first author2
  • middle author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.HE1
same name
  • J. Goldstein — 597 papers
  • J. Goldstein — 49 papers, h 87
  • J. Goldstein — 9 papers, h 10
  • J. Goldstein — 6 papers, h 5
  • J. Goldstein — 4 papers, h 33
  • J. Goldstein — 3 papers, h 34

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

activity
20142020
most citedAngular momentum transport by heat-driven g-modes in slowly pulsating B stars

208 citations · 396 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2020★ 75 cited

The Contour Method: a new approach to finding modes of non-adiabatic stellar pulsations

J. Goldstein, R. H. D. Townsend

The contour method is a new approach to calculating the non-adiabatic pulsation frequencies of stars. These frequencies can be found by solving for the complex roots of a character…

astro-ph.SR2018★ 16 cited

The Tayler Instability in the Anelastic Approximation

J. Goldstein, R. H. D. Townsend, E. G. Zweibel

The Tayler instability (TI) is a non-axisymmetric linear instability of an axisymmetric toroidal magnetic field in magneto-hydrostatic equilibrium (MHSE). Spruit (1999, 2002) has p…

astro-ph.SR2017★ 208 cited

Angular momentum transport by heat-driven g-modes in slowly pulsating B stars

R. H. D. Townsend, J. Goldstein, E. G. Zweibel

Motivated by recent interest in the phenomenon of waves transport in massive stars, we examine whether the heat-driven gravity (g) modes excited in slowly-pulsating B (SPB) stars c…

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