Hummel, W., Szeifert, T., Seifert, W., & Appenzeller, I. (2000). A spectroscopic study of Be stars in the SMC Cluster NGC 330. The Be phenomenon in early-type stars.
Chicago Style (17th ed.) CitationHummel, Wolfgang, Thomas Szeifert, Walter Seifert, and Immo Appenzeller. "A Spectroscopic Study of Be Stars in the SMC Cluster NGC 330." The Be Phenomenon in Early-type Stars 2000.
MLA (9th ed.) CitationHummel, Wolfgang, et al. "A Spectroscopic Study of Be Stars in the SMC Cluster NGC 330." The Be Phenomenon in Early-type Stars, 2000.
Warning: These citations may not always be 100% accurate.