A response to P.S. Conti's comment on "a three-dimensional classification for WN stars"

New Astronomy

Volumn 5, Issue 7, 2000, Pages 423-425

  Smith, Lindsey F ^a   Shara, Michael ^b   Moffat, Anthony ^c  

^a UNIVERSITY OF SYDNEY   (Australia)

^b DIVISION OF INVERTEBRATE ZOOLOGY   (United States)

^c UNIVERSITÉ DE MONTRÉAL   (Canada)

Author keywords

97.10.Ex; 97.10.Me; 97.10.Ri; Stars: fundamental parameters; Stars: Wolf Rayet

Indexed keywords

EID: 0141981253     PISSN: 13841076     EISSN: None     Source Type: Journal    
DOI: 10.1016/S1384-1076(00)00043-9     Document Type: Article

References (7)

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4. Hiltner, W.A. & Schild, R.E., 1966, ApJ, 143, 770.
5. Shara, M.M., Moffat, A.F.J., Smith, L.F., Niemela, V.S., Potter, M., & Lamontagne, R., 1999, AJ, 118, 390.
6. Smith, L.F., Shara, M.M. & Moffat, A.F.J., 1995, in: van der Hucht, K.A., Williams, P., (Eds.), Proc. IAU Symp. 163, Wolf-Rayet stars: binaries, colliding winds, evolution, Reidel, Dordrecht, p. 48.
7. Smith, L.F., Shara, M.M. & Moffat, A.F.J., 1996, MNRAS, 281, 163.