Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-23T03:34:10.115Z Has data issue: false hasContentIssue false
  • English
  • Français

LACEwING: Lessons from a New Moving Group Code

Published online by Cambridge University Press:  27 January 2016

A. R. Riedel
A. R. Riedel*
Affiliation:
The College of Staten Island email: adric.riedel@csi.cuny.eduCUNY-The College of Staten Island Hunter College, The American Museum of Natural History
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

With the recent accelerating rate of discoveries in the field of nearby young stars, the ability to identify new nearby young stars is as important as ever, and membership identification codes will continue to perform a vital role in scientific research. In the process of creating a new moving group membership identification code - LocAting Constituent mEmbers In Nearby Groups (LACEwING): we have compiled a few pointers relevant to astronomers trying to use codes like LACEwING to locate young stars.

Keywords

stars:low-massstars:pre-main-sequencegalaxy:open clusters and associations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S314: Young Stars & Planets Near the Sun , November 2015 , pp. 33 - 36
Copyright
Copyright © International Astronomical Union 2016 

References

Gagné, J., Lafrenière, D., Doyon, R., Malo, L. & Artigau, È. 2014, ApJ, 783, 121Google Scholar
Malo, L., Doyon, R., & Lafrenière, D.; et al. 2013, ApJ, 762, 88Google Scholar
Murphy, S. J. & Lawson, W. A. 2015, MNRAS, 447, 1267CrossRefGoogle Scholar
Riedel, A.R., Blunt, S.C., Rice, E.L. et al. submitted, ApJGoogle Scholar
Rodriguez, D. R., Zuckerman, B., Kastern, J. H., et al. 2013, ApJ, 774, 101Google Scholar