output
19942026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

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70 papers · 1 filter

astro-ph.SR2024★ 12 cited

Binary properties of the globular cluster 47 Tuc (NGC 104). A dearth of short-period binaries

Johanna Müller-Horn, Fabian Göttgens, Stefan Dreizler +4

Spectroscopic observations of binary stars in globular clusters are essential to shed light on the poorly constrained period, eccentricity, and mass ratio distributions and to deve…

astro-ph.CO2024★ 3 cited

FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields

Lurdes Ondaro-Mallea, Raul E. Angulo, Giovanni Aricò +3

Most of the visible matter in the Universe is in a gaseous state, subject to hydrodynamic forces and galaxy formation processes that are much more complex to model than gravity. Th…

astro-ph.GA2024★ 8 cited

The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies

Elisa A. Tau, Antonela Monachesi, Facundo A. Gomez +7

The stellar halos of dwarf galaxies are becoming an object of interest in the extragalactic community due to their detection in some recent observations. Additionally, new cosmolog…

astro-ph.HE2024★ 9 cited

Multi-Peaked Non-Thermal Light Curves from Magnetar-Powered Gamma-Ray Bursts

Conor M. B. Omand, Nikhil Sarin, Gavin P. Lamb

Binary neutron star mergers and collapsing massive stars can both create millisecond magnetars. Such magnetars are candidate engines to power gamma-ray bursts (GRBs). The non-therm…

astro-ph.GA2024★ 5 cited

Interaction between the Supernova Remnant W44 and the Infrared Dark Cloud G034.77-00.55: shock induced star formation?

G. Cosentino, I. Jiménez-Serra, A. T. Barnes +11

How Supernova Remnant (SNR) shocks impact nearby molecular clouds is still poorly observationally constrained. It is unclear if SNRs can positively or negatively affect clouds star…

astro-ph.HE2024★ 4 cited

Multi-wavelength study of OT 081: broadband modelling of a transitional blazar

MAGIC Collaboration, H. Abe, S. Abe +270

OT 081 is a well-known, luminous blazar that is remarkably variable in many energy bands. We present the first broadband study of the source which includes very-high-energy (VHE, $…