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)
- Institution
- The University of North Carolina at Greensboro (UNCG )
- Web Site: http://library.uncg.edu/
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.
The pre-main-sequence star IP Persei
PDF (Portable Document Format)
1535 KB
Created on 1/1/2001
Views: 2495
Additional Information
- Publication
- Astronomy and Astrophysics 377, 854-867
- Language: English
- Date: 2001
- Keywords
- stars: emission-line, stars: pre-main-sequence, stars: individual IP Per, techniques: spectroscopic, techniques photometric