602 citations
- Centre National de la Recherche ScientifiqueFR11 papers
- Utrecht UniversityNL9 papers
- International Solvay InstitutesBE8 papers
- Université Libre de BruxellesBE8 papers
- European Organization for Nuclear ResearchCH7 papers
- Johannes Gutenberg University MainzDE7 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR6 papers
- Evgeni Kharadze Georgian National Astrophysical ObservatoryGE5 papers
- Institut Laue-LangevinFR5 papers
- Radboud University NijmegenNL5 papers
- Universitat de BarcelonaES5 papers
- University of ViennaAT5 papers
6 papers · 2 filters
Giants in the globular cluster omega Centauri: dust production, mass loss and distance
Iain McDonald, Jacco Th. van Loon, Leen Decin +5
We present spectral energy distribution modelling of 6875 stars in omega Centauri, obtaining stellar luminosities and temperatures by fitting literature photometry to state-of-the-…
Linear wave propagation in relativistic magnetohydrodynamics
R. Keppens, Z. Meliani
The properties of linear Alfvén, slow, and fast magnetoacoustic waves for uniform plasmas in relativistic magnetohydrodynamics (MHD) are discussed, augmenting the well-known expres…
Detectability of Gravitational Waves from Phase Transitions
Tina Kahniashvili, Arthur Kosowsky, Grigol Gogoberidze +1
Gravitational waves potentially represent our only direct probe of the universe when it was less than one second old. In particular, first-order phase transitions in the early univ…
Pushing the precision limit of ground-based eclipse photometry
M. Gillon, D. R. Anderson, B. -O. Demory +4
Until recently, it was considered by many that ground-based photometry could not reach the high cadence sub-mmag regime because of the presence of the atmosphere. Indeed, high freq…
The Structure of Protoplanetary Disks Surrounding Three Young Intermediate Mass Stars. I. Resolving the disk rotation in the [OI] 6300 Åline
G. van der Plas, M. E. van den Ancker, D. Fedele +4
We present high spectral resolution optical spectra of three young intermediate mass stars, in all of which we spectrally resolve the 6300 Angstrom [OI] emission line. Two of these…
Gravitational Radiation from Primordial Helical MHD Turbulence
Tina Kahniashvili, Grigol Gogoberidze, Bharat Ratra
We consider gravitational waves (GWs) generated by primordial inverse-cascade helical magneto-hydrodynamical (MHD) turbulence produced by bubble collisions at the electroweak phase…