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Study of the Wolf-Rayet population in NGC 604 using bi-dimensional spectroscopy

  • Jesús Maíz-Apellániz (a1) (a2), José Miguel Mas-Hesse (a1) and Enrique Pérez (a3)

Abstract

We study the properties of the young population of NGC 604 and find evidences for 1–2 Myr differences between different regions. Four of the eleven WR stars in NGC 604 are found to have wide Hα emission lines. None of the WR stars is located within knots of high density, high excitation gas, as opposed to some of the O-type stars.

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References

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Drissen, L., Moffat, A.F.J., Shara, M.M. 1993, AJ 105, 1400
Maíz-Apellániz, J., Mas-Hesse, J.M., Muñoz-Tuñón, C., Vilchez, J.M., Castañeda, H.O. 1998, A&A 329, 409
Terlevich, E., Díaz, Á.I., Terlevich, R., González-Delgado, R.M., Perez, E., Garcia Vargas, M.L. 1996, MNRAS 279, 1219
Wilson, C.D., Scoville, N. 1992, ApJ 385, 512

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