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researcher

Peter Kosec

6 papers here

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

author position
  • first author2
  • middle author3
  • last author1

Across the 6 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
  • astro-ph.GA2
ORCID 0000-0003-4511-8427

identity via Semantic Scholar / OpenAlex

activity
20142023
most citedOrigin of central abundances in the hot intra-cluster medium - II. Chemical enrichment and supernova yield models

68 citations · 135 across the 6 of their papers we have counts for

collaborators
Showing 2022Show all

3 papers · 1 filter

astro-ph.HE2022★ 11 cited

Unveiling the disc structure in ultraluminous X-ray source NGC 55 ULX-1

F. Barra, C. Pinto, D. J. Walton +11

Despite two decades of studies, it is still not clear whether ULX spectral transitions are due to stochastic variability in the wind or variations in the accretion rate or in the s…

astro-ph.HE2022★ 9 cited

The long stare at Hercules X-1 -- I. Emission lines from the outer disk, the magnetosphere boundary and the accretion curtain

P. Kosec, E. Kara, A. C. Fabian +11

Hercules X-1 is a nearly edge-on accreting X-ray pulsar with a warped accretion disk, precessing with a period of about 35 days. The disk precession allows for unique and changing…

astro-ph.HE2022★ 6 cited

A transient ultraluminous X-ray source in NGC 55

A. Robba, C. Pinto, F. Pintore +14

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 1039 erg s−1. The average number of ULXs per galaxy is still not…

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