gaia clusters
Posted: 12.06.2017, 20:36
A paper has been published which discusses the improvement in determining memberships of various Open Clusters when using Gaia data.
See http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query? ... ..19G&db_key=AST&nosetcookie=1
I've created a Celestia Addon which can be used to view the clusters and their memberships.
It's available at https://www.classe.cornell.edu/~seb/celestia/files/gaia_clusters.zip (8 MB, expands to 10.5 MB)
Here's a screengrab showing Open Cluster members as described in the paper:
For comparison, here's a picture taken from the same viewpoint using previously published cluster memberships which had been determined using pre-Gaia data.
The use of Gaia data produces results which are greatly improved for clusters which are reasonably close to us, but the kinematics and positions for more distant clusters obviously have room for improvement.
See http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query? ... ..19G&db_key=AST&nosetcookie=1
I've created a Celestia Addon which can be used to view the clusters and their memberships.
It's available at https://www.classe.cornell.edu/~seb/celestia/files/gaia_clusters.zip (8 MB, expands to 10.5 MB)
Here's a screengrab showing Open Cluster members as described in the paper:
For comparison, here's a picture taken from the same viewpoint using previously published cluster memberships which had been determined using pre-Gaia data.
The use of Gaia data produces results which are greatly improved for clusters which are reasonably close to us, but the kinematics and positions for more distant clusters obviously have room for improvement.