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D. Ségransan

3 papers here

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author position
  • middle author1
  • last author2

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

fields
  • astro-ph3
same name
  • D. Ségransan — 2 papers

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

most citedMetallicity of M dwarfs I. A photometric calibration and impact on the mass-luminosity relation at the bottom of the main sequence

19 citations · 19 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph2005★ 19 cited

Metallicity of M dwarfs I. A photometric calibration and impact on the mass-luminosity relation at the bottom of the main sequence

X. Bonfils, X. Delfosse, S. Udry +3

We obtained high resolution ELODIE and CORALIE spectra for both components of 20 wide visual binaries composed of an F-, G- or K-dwarf primary and an M-dwarf secondary. We analyse…

astro-ph2003

Modeling of Alpha Cen and Procyon using VLTI observations

P. Kervella, F. Thevenin, P. Morel +4

We present a novel approach to model the nearby stars Alpha Cen A & B and Procyon A using asteroseismic and interferometric constraints. Using the VINCI instrument installed at the…

astro-ph2003

VINCI / VLTI observations of Main Sequence stars

P. Kervella, F. Thevenin, P. Morel +7

Main Sequence (MS) stars are by far the most numerous class in the Universe. They are often somewhat neglected as they are relatively quiet objects (but exceptions exist), though t…

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