Is this project an undergraduate, graduate, or faculty project?

Undergraduate

Project Type

group

Campus

Daytona Beach

Authors' Class Standing

Alisa Tiselska, Senior Allyson Woodruff, P.h.D candidate

Lead Presenter's Name

Alisa Tiselska

Lead Presenter's College

DB College of Arts and Sciences

Faculty Mentor Name

Dr. Ted von Hippel

Abstract

We are developing a technique to determine the age of formation of the Galactic thin and thick disks based on the properties of white dwarfs. To achieve this goal, we calculated the U, V, and W velocity components for thousands of white dwarfs with parallaxes and proper motions from Gaia, yet without radial velocities. With a missing component of the space velocity and overlap in the UVW distributions of these three stellar populations, we determine probabilities that each white dwarfs belongs to one of these Galactic populations. We classified 101,418 likely thin disk white dwarfs, 3158 likely thick disk white dwarfs, and six halo candidates. We apply the BASE-9 Astro statistics software to derive ages and masses for each white dwarf, then explore the age distributions for each population.

Did this research project receive funding support (Spark, SURF, Research Abroad, Student Internal Grants, Collaborative, Climbing, or Ignite Grants) from the Office of Undergraduate Research?

Yes, Spark Grant

Share

COinS
 

Ages of White Dwarf Stars

We are developing a technique to determine the age of formation of the Galactic thin and thick disks based on the properties of white dwarfs. To achieve this goal, we calculated the U, V, and W velocity components for thousands of white dwarfs with parallaxes and proper motions from Gaia, yet without radial velocities. With a missing component of the space velocity and overlap in the UVW distributions of these three stellar populations, we determine probabilities that each white dwarfs belongs to one of these Galactic populations. We classified 101,418 likely thin disk white dwarfs, 3158 likely thick disk white dwarfs, and six halo candidates. We apply the BASE-9 Astro statistics software to derive ages and masses for each white dwarf, then explore the age distributions for each population.

 

To view the content in your browser, please download Adobe Reader or, alternately,
you may Download the file to your hard drive.

NOTE: The latest versions of Adobe Reader do not support viewing PDF files within Firefox on Mac OS and if you are using a modern (Intel) Mac, there is no official plugin for viewing PDF files within the browser window.