Photometry and Spectroscopy of Old, Outer Disk Star Clusters: vdB-Hagen 176, Berkeley 29 and Saurer 1

Clicks: 11
ID: 283048
2005
Free PDF
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This article has not been analysed, so there is no overall score — reader engagement is measured and shown alongside.
AI Quality Assessment
Not analyzed
Readership in this journal
Star

Ranked #802 of 803 articles by views in arXiv

Most read Least read

Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 803 in total.

Mint this article as an NFT
Not yet minted

Create a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.

5 SUSD one-off · no wallet required
Sign in to mint
Abstract
It has been previously proposed that some distant open clusters in the Milky Way may have been accreted during a dwarf galaxy merger, perhaps associated with the same event that led to the formation of the Galactic anticenter stellar structure (GASS), also known as the ``Monoceros Ring''. We have obtained VI and Washington+DDO51 photometric and medium resolution (R ~ 8000) multi-fiber spectroscopic data for the three distant old open clusters Berkeley 29, Saurer 1, and vdB-Hagen 176 (BH 176). These clusters are spatially coincident with GASS, but radial velocities and spectroscopic metallicities had not been available during previous studies of the GASS candidate cluster system. Similar data for the clusters Berkeley 20 and Berkeley 39 have been obtained for calibration purposes. We provide the first {\it reliable} radial velocity for BH 176 (V_{helio} = 11.2 +/- 5.3 km/s). We also find that V_{helio} = +95.4 +/- 3.6 and +28.4 +/- 3.6 km/s, for Saurer 1(A) and Berkeley 29, respectively. We show that alpha-enhanced isochrones, while spectroscopically motivated, provide a poor fit to Be29 in contrast to previous findings. We find that the clusters Berkeley 29 and Saurer 1 are consistent with the previously reported characteristics for GASS candidate clustersand the GASS stellar stream as derived from M-giant observations. However, the radial velocity and photometric metallicity ([Fe/H] ~ 0.0 dex) for BH 176 suggests that a connection of this cluster with the putative GASS cluster system is unlikely. We reassess the age-metallicity relation for the most likely members of the GASS clusters system for which spectroscopic metallicities are now available.
Reference Key
kunkel2005photometry Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Peter M. Frinchaboy; Ricardo R. Munoz; Randy L. Phelps; Steven R. Majewski; William E. Kunkel
Journal arXiv
Year 2005
DOI
DOI not found
URL
http://arxiv.org/abs/astro-ph/0509742v1
Keywords
astro-ph

Citations

No citations found. To add a citation, contact the admin at info@scimatic.org

Comments

No comments yet. Be the first to comment on this article.