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C. M. Diez

3 papers here

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

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
ORCID 0000-0001-6520-4600
same name
  • C. M. Diez — 3 papers, h 4

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

most citedVariable structures in the stellar wind of the HMXB Vela X-1

5 citations · 6 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2025★ 3 cited

Dimming GRS 1915+105 observed with NICER and Insight--HXMT

M. Zhou, V. Grinberg, A. Santangelo +6

The black hole X-ray binary GRS 1915+105 was bright for 26 years since its discovery and is well-known for its disk instabilities, quasi-periodic oscillations, and disk wind signat…

astro-ph.HE2024

Multiwavelength study of 1eRASS J085039.9-421151 with eROSITA NuSTAR and X-shooter

Aafia Zainab, Artur Avakyan, Victor Doroshenko +23

The eROSITA instrument on board Spectrum-Roentgen-Gamma has completed four scans of the X-ray sky, leading to the detection of almost one million X-ray sources in eRASS1 only, incl…

astro-ph.HE2024★ 5 cited

Variable structures in the stellar wind of the HMXB Vela X-1

L. Abalo, P. Kretschmar, F. Fürst +9

Strong stellar winds are an important feature in wind-accreting high-mass X-ray binary (HMXB) systems, providing insights into stellar evolution and their impact on surrounding env…

astro-ph.HE2024★ 1 cited

Characterisation of the stellar wind in Cyg X-1 via modelling of colour-colour diagrams

E. V. Lai, B. De Marco, Y. Cavecchi +11

Cygnus X-1 is a high mass X-ray binary where accretion onto the black hole is mediated by the stellar wind from the blue supergiant companion star HDE 226868. Depending on the posi…

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