pith. machine review for the scientific record. sign in

arxiv: 1611.02687 · v1 · pith:UMB7EEXFnew · submitted 2016-11-08 · 🌌 astro-ph.SR · astro-ph.GA

White Dwarfs in the Metal-Rich Open Cluster NGC 6253

classification 🌌 astro-ph.SR astro-ph.GA
keywords clusterwhitedwarfsimagesdwarffilterhighmetal
0
0 comments X
read the original abstract

We have obtained 53 images with the $g$ filter and 19 images with the $i$ filter, each with 600-second exposures of the super metal rich open cluster NGC 6253 with the Gemini-South telescope to create deep images of the cluster to observe the cluster white dwarfs for the first time. We will analyze the white dwarf luminosity function to measure the cluster's white dwarf age, search for any anomalous features (as has been seen in the similarly metal rich cluster NGC 6791), and constrain the initial-final mass relation at high metallicities. We present an update on these observations and our program to study the formation of white dwarfs in super high metallicity environments.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.