496 citations
- Planetary Science InstituteUS47 papers
- University of ArizonaUS44 papers
- Ames Research CenterUS33 papers
- Jet Propulsion LaboratoryUS32 papers
- Southwest Research InstituteUS32 papers
- Johns Hopkins University Applied Physics LaboratoryUS24 papers
- Centre National de la Recherche ScientifiqueFR23 papers
- Goddard Space Flight CenterUS23 papers
- Search for Extraterrestrial IntelligenceUS22 papers
- Massachusetts Institute of TechnologyUS21 papers
- Lowell ObservatoryUS20 papers
- National Aeronautics and Space AdministrationUS17 papers
128 papers
Cometary ion dynamics at a weakly outgassing comet
Victor Steinwand, Peter Stephenson, Zoe Lewis +3
The ESA/Rosetta mission escorted comet 67P/Churyumov-Gerasimenko for two years, exploring its plasma environment across diverse outgassing conditions. Plasma density observations f…
Mare versus highland lunar impact flash light curve dichotomy
D. Athanasopoulos, A. Liakos, A. Z. Bonanos +5
We perform a comprehensive analysis of lunar impact flash (LIF) light curve shapes and their dependence on the lunar terrain, using the large sample of LIFs detected by NELIOTA ove…
X-Shooter survey of disk accretion in Upper Scorpius II. A lack of correlation between accretion rates and disk properties
A. Empey, C. F. Manara, R. Garcia Lopez +19
The evolution of protoplanetary discs is intertwined with the process of planet formation, growth and migration. Studies of nearby star forming regions of different ages and proper…
ExoplaNeT accRetion mOnitoring sPectroscopic surveY (ENTROPY) III. Optical He I line profiles of the accreting super Jupiter Delorme 1 (AB)b
Gayathri Viswanath, Mickaël Bonnefoy, Catherine Dougados +8
High-resolution spectroscopic observations of helium emission lines provide a powerful probe of accretion geometry in classical T Tauri stars, revealing regions not well traced by…
Benchmarking pre-main sequence stellar evolutionary tracks using disk-based dynamical stellar masses
Luigi Zallio, Miguel Vioque, Sean M. Andrews +14
Stellar masses are a fundamental property to understand models of pre-main sequence evolution, but their values derived from Hertzsprung-Russell (HR) diagrams are strongly model de…
The GAPS Programme at the TNG: LXX. TOI-5734b: A hot sub-Neptune orbiting a relatively young K dwarf with an Earth-like density
S. Filomeno, T. Trifonov, M. Damasso +40
Increasing interest in young exoplanets is leading to a growing effort to understand the formation and evolutionary processes responsible for their different architectures. One int…