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researcher

S. J. Qian

5 papers here

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

author position
  • sole author5

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.HE2
same name
  • S. J. Qian — 144 papers
  • S. J. Qian — 5 papers
  • S. J. Qian — 3 papers
  • S. J. Qian — 3 papers
  • S. J. Qian — 3 papers
  • S. J. Qian — 3 papers

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
20222024
collaborators

5 papers

astro-ph.HE2024

On a precessing jet-nozzle scenario with a common helical trajectory-pattern for blazar 3C345

S. J. Qian

The kinematics and flux evolution of the superluminal knots in blazar 3C345 were interpreted in the framework of the precessing jet-nozzle scenario with a precessing common helical…

astro-ph.GA2023

Flux evolution and kinematics of superluminal components in blazar 3C345

S. J. Qian

The precessing jet-nozzle scenario previously proposed was applied to model-fit the kinematics of five superluminal components (C19,C20,C21,B5 and B7) of jet-B in blazar 3C345. Bas…

astro-ph.HE2023

Flux evolution of superluminal components in blazar 3C454.3

S. J. Qian

The kinematic behavior of superluminal components observed at 43 GHz in blazar 3C454.3 were model-fitted with their light curves interpreted in terms of their Doppler-boosting effe…

astro-ph.GA2023

Kinematics and flux evolution of superluminal components in QSO B1308+326

S. J. Qian

Search for Doppler-boosting effect in flux evolution of superluminal components in blazars has been an important subject, which can help clarify their kinematic and emission proper…

astro-ph.GA2022

Doppler boosting effect and flux evolution of superluminal components in QSO 3C345

S. J. Qian

The precessing jet-nozzle scenario previously proposed was applied to interpret the VLBI-measured kinematics of five superluminal components (C4,C5,C9,C10 and C22) and their flux d…

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