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Saurabh Sharma

Panjab University, Chandigarh

21 papers hereh-index 3910.8k citations472 works total

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

author position
  • first author4
  • middle author6
  • last author2

Across the 12 of 21 papers where every author was matched, so the position is known.

fields
  • nucl-ex8
  • cs.CV5
  • astro-ph.SR4
  • astro-ph.GA3
  • cs.CL1
affiliations
  • Panjab University, Chandigarh
same name
  • Saurabh Sharma — 62 papers, h 16
  • Saurabh Sharma — 14 papers, h 4
  • Saurabh Sharma — 7 papers, h 1
  • Saurabh Sharma — 6 papers, h 2
  • Saurabh Sharma — 4 papers, h 3
  • Saurabh Sharma — 3 papers, 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
20142023
most citedBeam Energy Dependence of Triton Production and Yield Ratio (Nt​×Np​/Nd2​) in Au+Au Collisions at RHIC

52 citations · 240 across the 19 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2023

Fragmentation and dynamics of dense gas structures in the proximity of massive young stellar object W42-MME

N. K. Bhadari, L. K. Dewangan, L. E. Pirogov +4

We present an analysis of the dense gas structures in the immediate surroundings of the massive young stellar object (MYSO) W42-MME, using the high-resolution (0′′.31×0$''…

astro-ph.GA2023★ 1 cited

New insights in the bubble wall of NGC 3324: intertwined sub-structures and a bipolar morphology uncovered by JWST

L. K. Dewangan, A. K. Maity, Y. D. Mayya +4

We report the discovery of intertwined/entangled sub-structures towards the bubble wall of NGC 3324 below a physical scale of 4500 AU, which is the sharp edge/ionization front/elon…

astro-ph.GA2023

Dissecting the morphology of star forming complex S193

Rakesh Pandey, Saurabh Sharma, Lokesh Dewangan +5

We have studied a star-forming complex S193 using near-infrared (NIR) observations and other archival data covering optical to radio wavelengths. We identified stellar clusters in…

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