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New Emission-Line Stars in OH Clouds

Authors: G. L. Grasdalen; L. V. Kuhi; E. A. Harlan;

New Emission-Line Stars in OH Clouds

Abstract

Eleven dust clouds exhibiting radio OH lines have been surveyed for Ha emission-line stars. Eight new objects were discovered in four such clouds and none in the remaining seven to a limiting magnitude of m 18. The objects are most likely T Tauri stars. Key words: Ha-emission objects - T Tauri stars - OH emission - dust clouds

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Powered by OpenAIRE graph
Found an issue? Give us feedback
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
4
Average
Average
Average
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