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researcher

M. Clavel

57 papers hereh-index 211.4k citations95 works total

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

author position
  • first author3
  • middle author42
  • last author4

Across the 49 of 57 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE57
same name
  • M. Clavel — 6 papers, h 3
  • M. Clavel — 6 papers, h 3
  • M. Clavel — 3 papers, h 28
  • M. Clavel — 2 papers
  • M. Clavel — 1 paper, h 1
  • M. Clavel — 1 paper, h 1

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
20132026
most citedAlternative explanations for extreme supersolar iron abundances inferred from the energy spectrum of Cygnus X-1

142 citations · 2.2k across the 57 of their papers we have counts for

collaborators
Showing 2022Show all

3 papers · 1 filter

astro-ph.HE2022★ 15 cited

Absorption lines from magnetically driven winds in X-ray binaries II: high resolution observational signatures expected from future X-ray observatories

Susmita Chakravorty, Pierre-Olivier Petrucci, Sudeb Ranjan Datta +12

In our self-similar, analytical, magneto-hydrodynamic (MHD) accretion-ejection solution, the density at the base of the outflow is explicitly dependent on the disk accretion rate -…

astro-ph.HE2022★ 23 cited

Are Low-Frequency Quasi-Periodic Oscillations seen in accretion flows the disk response to a jet instability?

Jonathan Ferreira, Gregoire Marcel, Pierre-Olivier Petrucci +7

Low Frequency Quasi-Periodic Oscillations or LF QPOs are ubiquitous in BH X-ray binaries and provide strong constraints on the accretion-ejection processes. Although several models…

astro-ph.HE2022★ 12 cited

Classifying IGR J18007-4146 as an intermediate polar using XMM and NuSTAR

Benjamin M. Coughenour, John A. Tomsick, Aarran W. Shaw +5

Many new and unidentified Galactic sources have recently been revealed by ongoing hard X-ray surveys. A significant fraction of these have been shown to be the type of accreting wh…

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