Development of an H-Alpha Index for the Detection of PMS Candidates in Young Open Clusters
One phase of formation of medium- and low-mass stars is the optically visible phase known as the pre-main-sequence or PMS phase. In order to further the understanding of this phase, more of these PMS objects need to be identified and classified. Previous techniques have used photometry to identify p...
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| Format: | Others |
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BYU ScholarsArchive
2007
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| Online Access: | https://scholarsarchive.byu.edu/etd/1163 https://scholarsarchive.byu.edu/cgi/viewcontent.cgi?article=2162&context=etd |