7.1k citations
- L. Decin3 profiles136 · h 49
- C. Aerts3 profiles104 · h 67
- H. Sana3 profiles94 · h 44
- S. Poedts81 · h 46
- R. Keppens2 profiles70 · h 43
- T. Shenar61 · h 26
- A. de Koter2 profiles59 · h 12
- H. Van Winckel2 profiles59 · h 15
- B. Vandenbussche3 profiles58 · h 45
- D. Bowman46 · h 26
- A. Tkachenko2 profiles44 · h 26
- P. Lagage44 · h 45
- Centre National de la Recherche ScientifiqueFR488 papers
- Institute of AstronomyRU485 papers
- Université Paris CitéFR241 papers
- Radboud University NijmegenNL226 papers
- Sorbonne UniversitéFR209 papers
- Max Planck Institute for AstronomyDE194 papers
- University of AmsterdamNL190 papers
- Université Paris-SaclayFR189 papers
- Royal Observatory of BelgiumBE175 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR171 papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR160 papers
- Observatoire de ParisFR153 papers
30 papers · 2 filters
Coronal rain in magnetic arcades: Rebound shocks, Limit cycles, and Shear flows
X. Fang, C. Xia, R. Keppens +1
We extend our earlier multidimensional, magnetohydrodynamic simulations of coronal rain occurring in magnetic arcades with higher resolution, grid-adaptive computations covering a…
H2O vapor excitation in dusty AGB envelopes. A PACS view of OH 127.8+0.0
R. Lombaert, L. Decin, A. de Koter +6
Context: AGB stars lose a large percentage of their mass in a dust-driven wind. This creates a circumstellar envelope, which can be studied through thermal dust emission and molecu…
Population synthesis of classical low-mass X-ray binaries in the Galactic Bulge
L. M. van Haaften, G. Nelemans, R. Voss +2
Aims. We model the present-day population of 'classical' low-mass X-ray binaries (LMXBs) with neutron star accretors, which have hydrogen-rich donor stars. Their population is comp…
Solar prominences: 'double, double ... boil and bubble'
Rony Keppens, Chun Xia, Oliver Porth
Observations revealed rich dynamics within prominences, the cool 10,000 K, macroscopic (sizes of order 100 Mm) "clouds" in the million degree solar corona. Even quiescent prominenc…
IRAS 19135+3937: An SRd variable as interacting binary surrounded by a circumbinary disc
N. Gorlova, H. Van Winckel, N. P. Ikonnikova +6
Semi-regular (SR) variables are not a homogeneous class and their variability is often explained due to pulsations and/or binarity. This study focuses on IRAS 19135+3937, an SRd va…
Testing eccentricity pumping mechanisms to model eccentric long period sdB binaries with MESA
Joris Vos, Roy Østensen, Pablo Marchant +1
Hot subdwarf-B stars in long-period binaries are found to be on eccentric orbits, even though current binary-evolution theory predicts those objects to be circularised before the o…