Back to the Abstract

	1 Introduction
	2 The spectrum of Hu 1-2
	3 Chemical composition of the nebula
	4 Comparison with other abundance determinations
	5 The central star
	6 Recombination line radiation
	7 Discussion
	8 Summary and conclusion
	Appendix A: Visual lines
	Appendix B: Ultraviolet (IUE) lines
	References