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R. M. Ouazzani

3 papers here

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author position
  • first author1
  • middle author2

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

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  • astro-ph.SR3
ORCID 0000-0002-8586-5411

identity via Semantic Scholar / OpenAlex

most citedAngular momentum redistribution by mixed modes in evolved low-mass stars. II. Spin-down of the core of red giants induced by mixed modes

75 citations · 170 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2015★ 75 cited

Angular momentum redistribution by mixed modes in evolved low-mass stars. II. Spin-down of the core of red giants induced by mixed modes

K. Belkacem, J. P. Marques, M. J. Goupil +6

The detection of mixed modes in subgiants and red giants by the CoRoT and \emph{Kepler} space-borne missions allows us to investigate the internal structure of evolved low-mass sta…

astro-ph.SR2015★ 58 cited

Angular momentum redistribution by mixed modes in evolved low-mass stars. I. Theoretical formalism

K. Belkacem, J. P. Marques, M. J. Goupil +6

Seismic observations by the space-borne mission \emph{Kepler} have shown that the core of red giant stars slows down while evolving, requiring an efficient physical mechanism to ex…

astro-ph.SR2015★ 37 cited

Pulsations of rapidly rotating stars: II. Realistic modelling for intermediate-mass stars

Rhita-Maria Ouazzani, Ian W. Roxburgh, Marc-Antoine Dupret

Very high precision seismic space missions such as CoRoT and Kepler provide the means for testing the modelling of transport processes in stellar interiors. For some stars, such as…

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