26 citations
- CEA Paris-SaclayFR2 papers
- Centre National de la Recherche ScientifiqueFR2 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR2 papers
- Direction des EnergiesFR2 papers
- University of SouthamptonGB2 papers
- Canada–France–Hawaii TelescopeUS1 paper
- Goddard Space Flight CenterUS1 paper
- Institut de Planétologie et d'Astrophysique de GrenobleFR1 paper
- Institute of Astrophysics and Space SciencesPT1 paper
- Istituto di Astrofisica Spaziale e Fisica Cosmica di MilanoIT1 paper
- Max Planck Institute for Extraterrestrial PhysicsDE1 paper
- National Institute for AstrophysicsIT1 paper
5 papers · 1 filter
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…
Discovery of the INTEGRAL X/Gamma-ray transient IGR J00291+5934: a Comptonised accreting ms pulsar ?
S. E. Shaw, N. Mowlavi, J. Rodriguez +8
We report the discovery of a high-energy transient with the IBIS/ISGRI detector on board the INTEGRAL observatory. The source, namely IGR J00291+5934, was first detected on 2nd Dec…
Rotating massive stars: Pre-SN models and stellar yields at solar metallicity
R. Hirschi, G. Meynet, A. Maeder
We present a new set of stellar yields obtained from rotating stellar models at solar metallicity covering the massive star range (9-120 solar masses). The stellar models were calc…
INTEGRAL observations of the PSR B1259-63 / SS2883 system after the 2004 periastron passage
S. E. Shaw, M. Chernyakova, J. Rodriguez +3
The millisecond pulsar PSR B1259-63 and the Be star SS2883 are situated in a highly eccentric binary system, with orbital period ~3.4 years. We report on hard X-ray observations ob…
Quasar jet emission model applied to the microquasar GRS 1915+105
M. Turler, T. J. -L. Courvoisier, S. Chaty +1
The true nature of the radio emitting material observed to be moving relativistically in quasars and microquasars is still unclear. The microquasar community usually interprets the…