Asset Publisher

Siriusly, a newly identified intermediate-age Milky Way stellar cluster: A spectroscopic study of Gaia 1

Siriusly, a newly identified intermediate-age Milky Way stellar cluster: A spectroscopic study of Gaia 1

Publication date: 23 September 2017

Authors: J.D. Simpson, G.M. De Silva, S.L. Martell, D.B. Zucker, A.M.N. Ferguson, E.J. Bernard, M. Irwin, J. Penarrubia, & E. Tolstoy

Journal: Monthly Notices of the Royal Astronomical Society
Volume: 471
Issue: 4
Page: 4087-4098
Year: 2017

Copyright: © 2017 Oxford University Press

We confirm the reality of the recently discovered Milky Way stellar cluster Gaia 1 using spectra acquired with the HERMES and AAOmega spectrographs of the Anglo-Australian Telescope. This cluster had been previously undiscovered due to its close angular proximity to Sirius, the brightest star in the sky at visual wavelengths. Our observations identified 41 cluster members, and yielded an overall metallicity of [Fe/H]=−0.13±0.13 and barycentric radial velocity of vr = 58.30 ± 0.22 km s−1. These kinematics provide a dynamical mass estimate of 12.9+4.6−3.9×103M⊙ . Isochrone fits to Gaia, 2MASS, and Pan-STARRS1 photometry indicate that Gaia 1 is an intermediate age (∼3 Gyr) stellar cluster. Combining the spatial and kinematic data we calculate Gaia 1 has a circular orbit with a radius of about 12 kpc, but with a large out of plane motion: zmax=1.1+0.4−0.3  kpc. Clusters with such orbits are unlikely to survive long due to the number of plane passages they would experience.

Link to publication
Last Update: Sep 1, 2019 8:22:33 AM
21-Jan-2021 01:33 UT

ShortUrl Portlet

Shortcut URL

https://sci.esa.int/s/wKdZVrW

Images And Videos

Related Publications

Related Links

See Also

Documentation

Gaia EDR3 stories