The pre-main-sequence star IP Persei

UNCG Author/Contributor (non-UNCG co-authors, if there are any, appear on document)
Anatoly S. Miroshnichenko, Professor (Creator)
The University of North Carolina at Greensboro (UNCG )
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Abstract: We present the results of high- and low-resolution spectroscopic and broadband multicolour photometric observations of the emission-line A-type star IP Per. Significant variations of the Balmer line profiles and near-IR brightness are detected.

Additional Information

Astronomy and Astrophysics 377, 854-867
Language: English
Date: 2001
stars: emission-line, stars: pre-main-sequence, stars: individual IP Per, techniques: spectroscopic, techniques photometric

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