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Searching for Be Stars in the Open Cluster NGC663

Lee, C. D. and Yu, P. C. and Lin, C. C. and Chen, W. P. and Ip, W. H. and Ngeow, C. C. and Laher, Russ and Surace, Jason and Kulkarni, Shrinivas R. (2016) Searching for Be Stars in the Open Cluster NGC663. In: Bright Emissaries: Be Stars as Messengers of Star-disk Physics. Astronomical Society of the Pacific Conference Series. No.506. Astronomical Society of the Pacific , San Francisco, CA, pp. 271-274. ISBN 978-1-58381-896-1. https://resolver.caltech.edu/CaltechAUTHORS:20170608-111238343

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Abstract

With the Palomar Transient Factory Survey, we report Be stars candidates in the open cluster NGC 663, determined by Hα photometry which is to initiating a program to search for emission stars in clusters of different ages. We affirm the membership of these candidate by 2MASS magnitudes and colors, and by proper motions. Through the verifications, one known Be stars was ruled out because its inconsistent proper motions, and four new Be stars were discovered. More emission-line sources were also discovered, including non-member Be stars, dwarfs, and giants.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://aspbooks.org/a/volumes/article_details/?paper_id=37948PublisherArticle
ORCID:
AuthorORCID
Yu, P. C.0000-0001-8894-0854
Chen, W. P.0000-0003-0262-272X
Ip, W. H.0000-0002-3140-5014
Ngeow, C. C.0000-0001-8771-7554
Laher, Russ0000-0003-2451-5482
Surace, Jason0000-0001-7291-0087
Kulkarni, Shrinivas R.0000-0001-5390-8563
Additional Information:© 2016 Astronomical Society of the Pacific.
Group:Infrared Processing and Analysis Center (IPAC)
Series Name:Astronomical Society of the Pacific Conference Series
Issue or Number:506
Record Number:CaltechAUTHORS:20170608-111238343
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170608-111238343
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:78030
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:08 Jun 2017 21:38
Last Modified:19 Nov 2019 00:59

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