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researcher

G. Pavlov

120 papers hereh-index 425.7k citations364 works total

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

author position
  • first author16
  • middle author70
  • last author28

Across the 114 of 120 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE72
  • astro-ph45
  • astro-ph.GA2
  • physics.atom-ph1
same name
  • G. Pavlov — 105 papers, h 28
  • G. Pavlov — 35 papers, h 14
  • G. Pavlov — 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
19952023
most citedPulsar Wind Nebulae in the Chandra Era

211 citations · 5k across the 117 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.HE2023★ 5 cited

X-ray and near-infrared observations of the middle-aged pulsar B1055-52, its multiwavelength spectrum, and proper motion

B. Posselt, G. G. Pavlov, O. Kargaltsev +1

Previous observations of the middle-aged γ-ray, X-ray, and radio pulsar B1055-52 indicated some peculiarities, such as a suspected changing of the X-ray flux and spectral paramet…

astro-ph.HE2023★ 1 cited

First ejection from the PSR B1259-63/LS 2883 high mass gamma-ray binary detected during the 2021-2024 binary cycle

Jeremy Hare, George G. Pavlov, Oleg Kargaltsev +1

LS 2883/PSR B1259-63 is a high mass, eccentric gamma-ray binary that has previously been observed to eject X-ray emitting material. We report the results of recent Chandra observat…

astro-ph.HE2023★ 56 cited

Vela pulsar wind nebula x-rays are polarized to near the synchrotron limit

Fei Xie, Alessandro Di Marco, Fabio La Monaca +90

Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar…

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