Add to ORKGWe detected extended, curved stellar tidal tails emanating from the sparse, disrupting halo globular cluster Pal 5, which cover 10 degrees on the sky. These streams allow us to infer the orbit of Pal 5 and to ultimately constrain the Galactic potential at its location
We report the discovery of tidal tails around the two outer halo globular clusters, Eridanus and Pal...
In order to understand the extended massive tidal tails of the globular cluster Pal5, its very low m...
The tidal tails of Palomar 5 (Pal 5) have been the focus of many spectroscopic studies in an attempt...
We detected extended, curved stellar tidal tails emanating from the sparse, disrupting halo globular...
Using wide-field photometric data from the Sloan Digital Sky Survey (SDSS), we recently showed ...
Using wide-field photometric data from the Sloan Digital Sky Survey (SDSS) we recently showed that t...
We use photometry from the DECam Legacy Survey to detect candidate tidal tails extending ∼5° on eith...
Stars that escape globular clusters form tidal tails that are predominantly shaped by the global dis...
Sloan Digital Sky Survey data for the field of the cluster Pal 5 reveal the existence of a long mass...
Using the example of the tidal stream of the Milky Way globular cluster Palomar 5 (Pal 5), we demons...
The globular cluster Palomar 5 is remarkable not only because of its extended massive tidal tai...
We discuss recent observational and numerical work on tidal tails in globular clusters. Evidence of ...
Pal 5 is a low-mass, low-velocity-dispersion, globular cluster with spectacular tidal tails. We use ...
Using Data Release 4 of the Sloan Digital Sky Survey, we have applied an optimal contrast, matched f...
Using photometry and proper motions from Gaia Data Release 2, we detect a 50° long stream of about 7...
We report the discovery of tidal tails around the two outer halo globular clusters, Eridanus and Pal...
In order to understand the extended massive tidal tails of the globular cluster Pal5, its very low m...
The tidal tails of Palomar 5 (Pal 5) have been the focus of many spectroscopic studies in an attempt...
We detected extended, curved stellar tidal tails emanating from the sparse, disrupting halo globular...
Using wide-field photometric data from the Sloan Digital Sky Survey (SDSS), we recently showed ...
Using wide-field photometric data from the Sloan Digital Sky Survey (SDSS) we recently showed that t...
We use photometry from the DECam Legacy Survey to detect candidate tidal tails extending ∼5° on eith...
Stars that escape globular clusters form tidal tails that are predominantly shaped by the global dis...
Sloan Digital Sky Survey data for the field of the cluster Pal 5 reveal the existence of a long mass...
Using the example of the tidal stream of the Milky Way globular cluster Palomar 5 (Pal 5), we demons...
The globular cluster Palomar 5 is remarkable not only because of its extended massive tidal tai...
We discuss recent observational and numerical work on tidal tails in globular clusters. Evidence of ...
Pal 5 is a low-mass, low-velocity-dispersion, globular cluster with spectacular tidal tails. We use ...
Using Data Release 4 of the Sloan Digital Sky Survey, we have applied an optimal contrast, matched f...
Using photometry and proper motions from Gaia Data Release 2, we detect a 50° long stream of about 7...
We report the discovery of tidal tails around the two outer halo globular clusters, Eridanus and Pal...
In order to understand the extended massive tidal tails of the globular cluster Pal5, its very low m...
The tidal tails of Palomar 5 (Pal 5) have been the focus of many spectroscopic studies in an attempt...