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E. Steinberg

26 papers hereh-index 14601 citations31 works total

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

author position
  • first author11
  • middle author9
  • last author3

Across the 23 of 26 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE12
  • astro-ph.GA4
  • astro-ph.EP3
  • astro-ph.IM3
  • physics.comp-ph3
  • astro-ph.SR1
same name
  • E. Steinberg — 16 papers, h 18
  • E. Steinberg — 1 paper, h 4
  • E. Steinberg — 1 paper, h 2

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
20102023
most citedThe Galactic Center cloud G2 and its gas streamer

101 citations · 658 across the 24 of their papers we have counts for

collaborators
Showing 2014Show all

4 papers · 1 filter

astro-ph.IM2014★ 43 cited

Rich: Open Source Hydrodynamic Simulation on a Moving Voronoi Mesh

Almog Yalinewich, Elad Steinberg, Re'em Sari

We present here RICH, a state of the art 2D hydrodynamic code based on Godunov's method, on an unstructured moving mesh (the acronym stands for Racah Institute Computational Hydrod…

astro-ph.IM2014★ 3 cited

Balancing the load: A Voronoi based scheme for parallel computations

Elad Steinberg, Almog Yalinewich, Re'em Sari +1

The use of numerical simulations in science is ever increasing and with it the computational size. In many cases single processors are no longer adequate and simulations are run on…

astro-ph.GA2014★ 101 cited

The Galactic Center cloud G2 and its gas streamer

Oliver Pfuhl, Stefan Gillessen, Frank Eisenhauer +10

We present new, deep near-infrared SINFONI @ VLT integral field spectroscopy of the gas cloud G2 in the Galactic Center, from late summer 2013 and spring 2014. G2 is visible in rec…

astro-ph.EP2014

Spins of large asteroids: Hint on a primordial distribution of their spin rates

Elad Steinberg, Re'em Sari

The Asteroid Belt and the Kuiper Belt are relics from the formation of our solar system. Understanding the size and spin distribution of the two belts is crucial for a deeper under…

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