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M. Takata

4 papers hereh-index 277 citations4 works total

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

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
same name
  • M. Takata — 20 papers, h 91
  • M. Takata — 16 papers, h 15
  • M. Takata — 3 papers, h 6
  • M. Takata — 1 paper, h 8
  • M. Takata — 1 paper, h 3
  • M. Takata — 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
20162026
most citedDipole modes with depressed amplitudes in red giants are mixed modes

75 citations · 133 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2026

Extra modes in helium-core-burning stars probing an infra core cavity

B. Mosser, M. Takata, C. Pinçon +5

Dipole mixed modes observed in the oscillation pattern of red giant stars probe the radiative regions in the stellar core. Oscillation spectra of helium-core-burning stars sometime…

astro-ph.SR2023

Inferring coupling strengths of mixed-mode oscillations in red-giant stars using deep learning

Siddharth Dhanpal, Othman Benomar, Shravan Hanasoge +3

Asteroseismology is a powerful tool that may be applied to shed light on stellar interiors and stellar evolution. Mixed modes, behaving as acoustic waves in the envelope and buoyan…

astro-ph.SR2016★ 58 cited

Period spacings in red giants; III. Coupling factors of mixed modes

B. Mosser, C. Pinçon, K. Belkacem +2

The power of asteroseismology relies on the capability of global oscillations to infer the stellar structure. For evolved stars, we benefit from unique information directly carried…

astro-ph.SR2016★ 75 cited

Dipole modes with depressed amplitudes in red giants are mixed modes

B. Mosser, K. Belkacem, C. Pincon +6

Seismic observations have shown that a number of evolved stars exhibit low-amplitude dipole modes, which are referred to as depressed modes. Recently, these low amplitudes have bee…

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