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researcher

S. Krishna

4 papers hereh-index 343 citations5 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.GA3
  • astro-ph.SR1
same name
  • S. Krishna — 22 papers, h 16
  • S. Krishna — 8 papers, h 51
  • S. Krishna — 4 papers, h 4
  • S. Krishna — 2 papers, h 9
  • S. Krishna — 2 papers, h 3
  • S. Krishna — 2 papers, h 8

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
20172019
most citedPlanetary Nebulae with Ultra-Violet Imaging Telescope (UVIT): Far Ultra-violet halo around the Bow Tie nebula (NGC 40)

9 citations · 9 across the 1 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2018

Jets blowing bubbles in the young radio galaxy 4C 31.04

Henry R. M. Zovaro, Robert Sharp, Nicole P. H. Nesvadba +5

We report the discovery of shocked molecular and ionized gas resulting from jet-driven feedback in the compact radio galaxy 4C 31.04 using near-IR imaging spectroscopy. 4C 31.04 is…

astro-ph.GA2018

Planetary Nebulae with UVIT II: Revelations from FUV vision of Butterfly Nebula NGC 6302

N. Kameswara Rao, O. De Marco, S. Krishna +4

The high excitation planetary nebula, NGC 6302, has been imaged in two far-ultraviolet (FUV) filters, F169M (Sapphire; λeff​: 1608 Å) and F172M (Silica; λeff​: 1717…

astro-ph.GA2017★ 9 cited

Planetary Nebulae with Ultra-Violet Imaging Telescope (UVIT): Far Ultra-violet halo around the Bow Tie nebula (NGC 40)

N. Kameswara Rao, F. Sutaria, J. Murthy +3

Context. NGC 40 is a planetary nebula with diffuse X-ray emission, suggesting an interaction of the high speed wind from WC8 central star (CS) with the nebula. It shows strong Civ…

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