10.6k citations
- Centre National de la Recherche ScientifiqueFR6.9k papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR2.6k papers
- Université Paris Sciences et LettresFR2.5k papers
- Sorbonne UniversitéFR2.4k papers
- Université Paris DiderotFR2k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR1.7k papers
- Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresFR1.7k papers
- Université Paris CitéFR1.6k papers
- Galaxies, Etoiles, Physique et InstrumentationFR1.4k papers
- Université Pierre-et-Marie-CurieFR1.2k papers
- European Southern ObservatoryCL1.2k papers
- Sorbonne Paris CitéFR1.1k papers
1,947 papers · 1 filter
The MiMeS Project: Magnetism in Massive Stars
G. A. Wade, E. Alecian, D. A. Bohlender +11
The Magnetism in Massive Stars (MiMeS) Project is a consensus collaboration among the foremost international researchers of the physics of hot, massive stars, with the basic aim of…
Search for the magnetic field of the O7.5 III star xi Persei
H. F. Henrichs, R. S. Schnerr, J. A. de Jong +3
Cyclical wind variability is an ubiquitous but as yet unexplained feature among OB stars. The O7.5 III(n)((f)) star xi Persei is the brightest representative of this class on the N…
The magnetic field of the B3V star 16 Pegasi
H. F. Henrichs, C. Neiner, R. S. Schnerr +8
The Slowly Pulsating B3V star 16 Pegasi was discovered by Hubrig (2006) to be magnetic, based on low-resolution spectropolarimetric observations with FORS1 at the VLT. We have conf…
Discovery of non-radial pulsations in the spectroscopic binary Herbig Ae star RS Cha
T. Böhm, W. Zima, C. Catala +3
In this article we present a first discovery of non radial pulsations in both components of the Herbig Ae spectroscopic binary star RS Cha. The binary was monitored in quasi-contin…
The MiMeS Project: First Results
J. H. Grunhut, E. Alecian, D. A. Bohlender +11
Massive stars are those stars with initial masses above about 8 times that of the sun, eventually leading to catastrophic explosions in the form of supernovae. These represent the…
Discovery of fossil magnetic fields in the intermediate-mass pre-main sequence stars
E. Alecian, G. A. Wade, C. Catala
It is now well-known that the surface magnetic fields observed in cool, lower-mass stars on the main sequence (MS) are generated by dynamos operating in their convective envelopes.…