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Giovanni M. Mirouh

2 papers here

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author position
  • first author1
  • last author1

Across the 2 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
ORCID 0000-0003-0238-8435

identity via Semantic Scholar / OpenAlex

most citedDynamics of the photosphere along the solar cycle from SDO/HMI

5 citations · 5 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2023

The PL diagram for δ Sct stars: back in business as distance estimators

A. García Hernández, J. Pascual-Granado, M. Lares-Martiz +4

In this work, we focus on the period-luminosity relation (PLR) of δ Sct stars, in which mode excitation and selection mechanisms are still poorly constrained, and whose structure…

astro-ph.HE2023★ 24 cited

Population III X-ray Binaries and their Impact on the Early Universe

Nina S. Sartorio, A. Fialkov, T. Hartwig +8

The first population of X-ray binaries (XRBs) is expected to affect the thermal and ionization states of the gas in the early Universe. Although these X-ray sources are predicted t…

astro-ph.SR2016★ 5 cited

Dynamics of the photosphere along the solar cycle from SDO/HMI

Th. Roudier, J. M. Malherbe, G. M. Mirouh

As the global magnetic field of the Sun has an activity cycle, one expects to observe some variation of the dynamical properties of the flows visible in the photosphere. We investi…

astro-ph.SR2014

Gravito-inertial modes in a differentially rotating spherical shell

Giovanni M. Mirouh, Clément Baruteau, Michel Rieutord +1

Oscillations have been detected in a variety of stars, including intermediate- and high-mass main sequence stars. While many of these stars are rapidly and differentially rotating,…

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