434 citations
- F. Combes2 profiles16 · h 68
- C. Boisson2 profiles7 · h 64
- H. Sol4 profiles5 · h 62
- W. Benbow2 profiles5 · h 58
- B. Giebels2 profiles4 · h 83
- D. Emmanoulopoulos2 profiles4 · h 37
- G. Dubus2 profiles4 · h 64
- L. Costamante2 profiles4 · h 54
- M. Punch2 profiles4 · h 61
- M. Raue3 profiles4 · h 50
- O. Paris4 · h 54
- R. Samadi2 profiles4 · h 48
- Centre National de la Recherche ScientifiqueFR27 papers
- Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresFR25 papers
- Université Paris CitéFR17 papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR15 papers
- Sorbonne UniversitéFR15 papers
- Galaxies, Etoiles, Physique et InstrumentationFR10 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR8 papers
- Janssen (France)FR8 papers
- Observatoire de la Côte d’AzurFR8 papers
- Université de Versailles Saint-Quentin-en-YvelinesFR7 papers
- CEA Paris-SaclayFR6 papers
- Laboratoire AstroParticule et CosmologieFR6 papers
16 papers · 1 filter
Testing gravity on large scales. The skewness of the galaxy distribution at z~1
C. Marinoni, L. Guzzo, A. Cappi +54
We study the evolution of the low-order moments of the galaxy overdensity distribution over the redshift interval 0.7<z<1.5. We find that the variance and the normalized skewness e…
Pattern speed evolution and bar reformation
F. Combes
Bars in spiral galaxies can weaken through gas inflow towards the center, and angular momentum transfer. Several bar episodes can follow one another in the life of the galaxy, if s…
Multiline Zeeman signatures as demonstrated through the Pseudo-line
M. Semel, J. C. Ramirez Velez, M. J. Stift +3
In order to get a significant Zeeman signature in the polarised spectra of a magnetic star, we usually 'add' the contributions of numerous spectral lines; the ultimate goal is to r…
Stellar wobble caused by a binary system: Can it really be mistaken as an extra-solar planet?
Maria H. M. Morais, Alexandre C. M. Correia
The traditional method for detecting extra-solar planets relies on measuring a small stellar wobble which is assumed to be caused by a planet orbiting the star. Recently, it was su…
VLBI observations of jupiter with the initial test station of LOFAR and the nancay decametric array
A. Nigl, P. Zarka, J. Kuijpers +3
AIMS: To demonstrate and test the capability of the next generation of low-frequency radio telescopes to perform high resolution observations across intra-continental baselines. Ju…
Reference grids of stellar models and oscillation frequencies: Data from the CESAM stellar evolution code and ADIPLS oscillation programme
Yveline Lebreton, Eric Michel
We present grids of stellar models and their associated oscillation frequencies that have been used by the CoRoT Seismology Working Group during the scientific preparation of the C…