From the 6 of 215 papers with an AI index.
330 citations
- Sorbonne UniversitéFR70 papers
- Université Paris-SaclayFR61 papers
- Centre National de la Recherche ScientifiqueFR59 papers
- University of CambridgeGB58 papers
- University of ZurichCH58 papers
- University of Chinese Academy of SciencesCN57 papers
- Heidelberg UniversityDE56 papers
- University of Maryland, College ParkUS56 papers
- University of MichiganUS56 papers
- Aix-Marseille UniversitéFR55 papers
- Massachusetts Institute of TechnologyUS55 papers
- National Institute for Subatomic PhysicsNL55 papers
9 papers · 1 filter
The role of mass transfer efficiency in stability criteria: Implementation in SEVN and a test on blue stragglers and binary compact objects
M. Echeveste, G. J. Escobar, G. Iorio +12
Context: The stability of mass transfer through Roche-lobe overflow plays a key role in shaping the outcome of binary interactions. However, the criterion for mass transfer stabili…
XP-TEAL: Gaia XP tool for emission and absorption lines. I. Balmer lines in open clusters
J. M. Carrasco, M. Weiler, S. Malhotra +5
Context. The third Gaia data release (Gaia DR3) includes blue and red low-resolution spectrophotometry for more than 200 million sources. These Gaia XP spectra are represented by s…
Compact HII Regions as Clocks of Massive-Star Formation: Evidence for Long Formation Timescales
Paolo Padoan, Mark Gieles
We revisit the luminosity function (LF) of compact HII regions in the context of the inertial--inflow model (IIM), in which massive stars assemble over extended, mass-dependent tim…
Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion
Sergio A. Dzib, JazmÃn Ordóñez-Toro, Laurent Loinard +9
We present results from a multi-epoch Very Long Baseline Array (VLBA) survey conducted as part of the DYNAMO-VLBA project, aimed at measuring the dynamical masses of young stellar…
Extending TESS flare frequency distributions with CHEOPS: Power-law versus lognormal
Julien Poyatos, Octavi Fors, José Maria Gómez Cama
Stellar flares are intense bursts of radiation caused by magnetic reconnection on active stars. They are especially frequent on M dwarfs, where they can significantly influence the…
Dynamical masses of YSOs with the VLBA: DYNAMO VLBA: Trigonometric parallaxes and proper motions of YSOs in Orion
Sergio A. Dzib, JazmÃn Ordóñez-Toro, Laurent Loinard +9
We present results from a multi-epoch Very Long Baseline Array (VLBA) survey of compact radio sources in the Orion complex, conducted within both the DYNAMO-VLBA and the GOBELINS p…