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TOWARD UNDERSTANDING THE B[e] PHENOMENON. III. PROPERTIES OF THE OPTICAL COUNTERPART OF IRAS 00470+6429

A. S. Miroshnichenko,E. L. Chentsov,V. G. Klochkova,S. V. Zharikov,K. N. Grankin,A. V. Kusakin,T. L. Gandet,G. Klingenberg, S. Kildahl,R. J. Rudy,D. K. Lynch,C. C. Venturini,S. Mazuk,R. C. Puetter,R. B. Perry,A. C. Carciofi,K. S. Bjorkman,R. O. Gray,S. Bernabei,V. F. Polcaro,R. F. Viotti,L. Norci

The Astrophysical Journal（2009）

Cited 28|Views43
Key words
circumstellar matter,stars: early-type,stars: emission-line, Be,stars: individual (IRAS 00470+6429)
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