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830 documents correspondants.

Prépublication · 2026 arXiv EN

The origin of the large heavy element contents of warm Jupiters

Planet interior models have revealed that warm Jupiters should harbor large heavy element masses (up to 30-40% of the planetary mass). Within the pebble drift and evaporation scenario, inward drifting pebbles can evaporate and enrich the inner disc with vapor...

Bertram Bitsch #astro-ph.EP
Prépublication · 2026 arXiv EN

Assessing PLATO's Discovery Potential across Different Observing Strategies

The PLATO mission, planned to launch in spring 2027, will observe a fixed Southern field, LOPS2, for at least 2 years with the goal of discovering and deriving precise parameters for planets as small as Earth around FGK dwarfs and sub-giants. Afterwards, PLATO...

Yoshi Nike Emilia Eschen, Michelle Kunimoto et al. #astro-ph.EP
Prépublication · 2026 arXiv EN

How long could volcanic plumes persist in the Venus atmosphere?

Resolving the ambiguity surrounding current Venusian volcanism is a primary objective for upcoming missions like EnVision and VERITAS. This study uses the Venus Planetary Climate Model to simulate the dispersal and detectability of volcanic plumes containing w...

Maureen Cohen, James Holmes et al. #astro-ph.EP
Prépublication · 2026 arXiv EN

Detecting redshift space distortions with forthcoming 21cm intensity maps from MeerKLASS

Redshift space distortions (RSD) provide a powerful measurement of structure formation in modern cosmology. In this work, we explore the potential of 21cm intensity mapping with the MeerKAT Large Area Synoptic Survey (MeerKLASS) to detect RSD and probe gravity...

Daniel Tassie, Steven Cunnington et al. #astro-ph.CO
Prépublication · 2026 arXiv EN

Combination of multi-observatory photometry to determine asteroid rotation periods

This study aims to determine asteroid rotation periods from sparse, unevenly sampled, multi-observatory photometry using the Lomb-Scargle (L-S) method. The photometric measurements of the asteroids are taken from the circulars of the Minor Planet Center (MPC)....

Kristers Nagainis, Ilgmars Eglitis #astro-ph.EP
Prépublication · 2026 arXiv EN

Detailed study of HD 219134: a benchmark K-dwarf with a compact planetary system

Space missions such as CoRoT, Kepler, and TESS have transformed asteroseismology and its synergies with exoplanet science. We revisit the nearby K-dwarf HD 219134 to investigate the tension between asteroseismic and interferometric radii, update its fundamenta...

Jérôme Bétrisey, Camilla Pezzotti et al. #astro-ph.EP
Prépublication · 2026 arXiv EN

Star Cluster Ecology VIII. -- Dynamically Forming S-Type and $α$Centauri-like Systems

Aims: To analyse the impact of dynamically formed binaries emerging naturally from various star cluster environments on already established planetary systems. Methods: Numerical simulations replicating the star-forming region NGC 1333 are conducted. We conside...

Erwan Hochart, Simon Portegies Zwart #astro-ph.EP
Prépublication · 2026 arXiv EN

A Relationship Between Fast Radio Burst Dispersion Measure and Host Galaxy Inclination

It is commonly thought that fast radio bursts (FRBs) trace star formation, and that they are produced by magnetars. Both hypotheses imply that their sources are hosted primarily (but not exclusively) in galactic disks. Although there is evidence in that direct...

Lachlan Marnoch, Stuart D. Ryder et al. #astro-ph.GA