The GD-1 stream is one of the longest and coldest stellar streams discovered to date, and one of the best objects for constraining the dark matter properties of the Milky Way. Using data from Gaia DR2 we study the proper motions, distance, morphology and density of the streamto uncover small scale perturbations. The proper motion cleaned data shows a clear distance gradient across the stream, ranging from 7 to 12 kpc. However, unlike earlier studies thatfound a continuous gradient, we uncover a distance minimum atφ1≈-50 deg, after which the distance increases again. We can reliably trace the stream between -85< φ1<15 deg, show-ing an even further extent to GD-1 beyond the earlier extension of Price-Whelan & Bonaca(2018). We constrain the st...
International audienceSTREAMFINDER is a new algorithm that we have built to detect stellar streams i...
Cold stellar streams—produced by tidal disruptions of globular clusters—are long-lived, coherent dyn...
International audienceWe use ESA/Gaia astrometry together with SEGUE and LAMOST measurements of the ...
The GD-1 stream is one of the longest and coldest stellar streams discovered to date, and one of the...
We present a model for the interaction of the GD-1 stellar stream with a massive perturber that natu...
GD-1 is a long, thin, Milky Way star stream that has readily visible density variations along its le...
With the photometric data from the SDSS survey, the spectroscopic data from the SDSS/SEGUE and the L...
The longest recognized stellar stream in the Milky Way Galaxy has an expanse of over more than half ...
We investigate the effects of a massive ($\gtrsim4\times10^{10}M_\odot$) Sagittarius dwarf spheroida...
Context. The Sagittarius dwarf spheroidal (Sgr) is a dissolving galaxy being tidally disrupted by th...
International audienceContext. The Sagittarius dwarf spheroidal (Sgr) is a dissolving galaxy being t...
International audienceThe density variations in thin stellar streams may encode important informatio...
Stellar streams, the tidal remnants of accreted globular clusters and dwarf galaxies, are uniquely p...
The Sagittarius dwarf galaxy (Sgr) is a satellite that is currently being consumed by the Milky Way’...
The narrow GD-1 stream of stars, spanning 60ð on the sky at a distance of ~10 kpc from the Sun an...
International audienceSTREAMFINDER is a new algorithm that we have built to detect stellar streams i...
Cold stellar streams—produced by tidal disruptions of globular clusters—are long-lived, coherent dyn...
International audienceWe use ESA/Gaia astrometry together with SEGUE and LAMOST measurements of the ...
The GD-1 stream is one of the longest and coldest stellar streams discovered to date, and one of the...
We present a model for the interaction of the GD-1 stellar stream with a massive perturber that natu...
GD-1 is a long, thin, Milky Way star stream that has readily visible density variations along its le...
With the photometric data from the SDSS survey, the spectroscopic data from the SDSS/SEGUE and the L...
The longest recognized stellar stream in the Milky Way Galaxy has an expanse of over more than half ...
We investigate the effects of a massive ($\gtrsim4\times10^{10}M_\odot$) Sagittarius dwarf spheroida...
Context. The Sagittarius dwarf spheroidal (Sgr) is a dissolving galaxy being tidally disrupted by th...
International audienceContext. The Sagittarius dwarf spheroidal (Sgr) is a dissolving galaxy being t...
International audienceThe density variations in thin stellar streams may encode important informatio...
Stellar streams, the tidal remnants of accreted globular clusters and dwarf galaxies, are uniquely p...
The Sagittarius dwarf galaxy (Sgr) is a satellite that is currently being consumed by the Milky Way’...
The narrow GD-1 stream of stars, spanning 60ð on the sky at a distance of ~10 kpc from the Sun an...
International audienceSTREAMFINDER is a new algorithm that we have built to detect stellar streams i...
Cold stellar streams—produced by tidal disruptions of globular clusters—are long-lived, coherent dyn...
International audienceWe use ESA/Gaia astrometry together with SEGUE and LAMOST measurements of the ...