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researcher

V. Chavushyan

9 papers hereh-index 4156 citations10 works total

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

author position
  • middle author6
  • last author1

Across the 7 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO4
  • astro-ph.GA4
  • astro-ph1
same name
  • V. Chavushyan — 75 papers, h 26
  • V. Chavushyan — 25 papers, h 5
  • V. Chavushyan — 21 papers, h 11
  • V. Chavushyan — 19 papers, h 9
  • V. Chavushyan — 4 papers
  • V. Chavushyan — 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
20042016
most citedLong-term variability of the optical spectra of NGC 4151: II. Evolution of the broad Ha and Hb emission-line profiles

90 citations · 430 across the 9 of their papers we have counts for

collaborators
Showing 2009Show all

3 papers · 1 filter

astro-ph.GA2009★ 90 cited

Long-term variability of the optical spectra of NGC 4151: II. Evolution of the broad Ha and Hb emission-line profiles

A. I. Shapovalova, L. C. Popovic, A. N. Burenkov +5

Results of the long-term (11 years, from 1996 to 2006) Hα and Hβ line variations of the active galactic nucleus of NGC 4151 are presented. High quality spectra (S/N>50 and R~8A…

astro-ph.CO2009★ 50 cited

Relativistic plasma as the dominant source of the optical continuum emission in the broad-line radio galaxy 3C 120

J. Leon-Tavares, A. P. Lobanov, V. H. Chavushyan +5

We report a relation between radio emission in the inner jet of the Seyfert galaxy 3C 120 and optical continuum emission in this galaxy. Combining the optical variability data with…

astro-ph.CO2009★ 63 cited

Observational evidence for the link between the variable optical continuum and the subparsec-scale jet of the radio galaxy 3C 390.3

T. G. Arshakian, J. Leon-Tavares, A. P. Lobanov +4

The mechanism and the region of generation of variable continuum emission are poorly understood for radio-loud AGN because of a complexity of the nuclear region. High-resolution ra…

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