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researcher

S. Popov

127 papers hereh-index 252.1k citations182 works total

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

author position
  • sole author20
  • first author38
  • middle author23
  • last author34

Across the 115 of 127 papers where every author was matched, so the position is known.

fields
  • astro-ph57
  • astro-ph.HE54
  • gr-qc4
  • astro-ph.EP3
  • astro-ph.SR3
  • astro-ph.GA2
same name
  • S. Popov — 65 papers
  • S. Popov — 28 papers
  • S. Popov — 22 papers, h 29
  • S. Popov — 9 papers, h 3
  • S. Popov — 8 papers, h 11
  • S. Popov — 7 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 citedPopulation synthesis studies of isolated neutron stars with magnetic field decay

153 citations · 2.1k across the 124 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.HEShow all

4 papers · 2 filters

astro-ph.HE2012★ 26 cited

Jets and gamma-ray emission from isolated accreting black holes

M. V. Barkov, D. V. Khangulyan, S. B. Popov

The large number of isolated black holes (IBHs) in the Galaxy, estimated to be 10^8, implies a very high density of 10^-4 pc^-3 and an average distance between IBHs of 10 pc. Our s…

astro-ph.HE2012★ 48 cited

SXP 1062: an Evolved Magnetar in a BeXB ?

R. Turolla, S. B. Popov

SXP 1062, a newly discovered Be/X-ray binary in the Small Magellanic Cloud, provides the first example of a robust association with a supernova remnant (SNR). The short age estimat…

astro-ph.HE2012★ 3 cited

Initial parameters of neutron stars

S. B. Popov, R. Turolla

A subpopulation of neutron stars (NSs), known as central compact objects (CCOs) in supernova remnants, are suspected to be low-field objects basing on P-P˙ measurements for…

astro-ph.HE2012★ 91 cited

Initial spin periods of neutron stars in supernova remnants

S. B. Popov, R. Turolla

We present estimates of initial spin periods, P0​, for radio pulsars associated with supernova remnants. By using the published data on 30 objects, we were able to derive a relia…

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