Measuring the Distance to Low-Mass Star Forming Cores
ORAL
Abstract
The study of low-mass star formation has made great advances in the past decade with the advent of space and ground-based telescopes. However, the understanding of these regions is often hindered by a lack of knowledge of the star-forming cores' distance. We present a simple plan and preliminary results to determine the distance to areas of low-mass star formation.
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Authors
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Chadwick Young
Nicholls State University
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Leah Garber
Nicholls State University
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Tyler Bourke
Harvard-Smithsonian Center for Astrophysics