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researcher

T. Morel

33 papers hereh-index 10422 citations21 works total

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

author position
  • first author4
  • middle author19

Across the 23 of 33 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR30
  • astro-ph.GA2
  • astro-ph.EP1
same name
  • T. Morel — 75 papers, h 42
  • T. Morel — 11 papers, h 7
  • T. Morel — 4 papers, h 6
  • T. Morel — 3 papers
  • T. Morel — 3 papers, h 4
  • T. Morel — 3 papers, h 6

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
20092026
most citedRed-giant seismic properties analyzed with CoRoT

236 citations · 1.5k across the 33 of their papers we have counts for

collaborators
Showing 2010Show all

4 papers · 1 filter

astro-ph.SR2010★ 1 cited

Can an underestimation of opacity explain B-type pulsators in the SMC?

S. Salmon, J. Montalbán, A. Miglio +3

Slowly Pulsating B and β Cephei are κ mechanism driven pulsating B stars. That κ mechanism works since a peak in the opacity due to a high number of atomic transitions from i…

astro-ph.SR2010★ 16 cited

First orbital solution for the non-thermal emitter Cyg OB2 #9

Y. Naze, Y. Damerdji, G. Rauw +7

After the first detection of its binary nature, the spectroscopic monitoring of the non-thermal radio emitter Cyg OB2 #9 (P=2.4yrs) has continued, doubling the number of available…

astro-ph.SR2010★ 236 cited

Red-giant seismic properties analyzed with CoRoT

B. Mosser, K. Belkacem, M. J. Goupil +10

The CoRoT 5-month long observation runs give us the opportunity to analyze a large variety of red-giant stars and to derive fundamental stellar parameters from their asteroseismic…

astro-ph.SR2010★ 66 cited

Non-radial oscillations in the red giant HR7349 measured by CoRoT

F. Carrier, J. De Ridder, F. Baudin +13

Convection in red giant stars excites resonant acoustic waves whose frequencies depend on the sound speed inside the star, which in turn depends on the properties of the stellar in…

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