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The abundance gradient across M 81GARNETT, D. R.Publications of the Astronomical Society of the Pacific. 1986, Vol 98, Num 608, pp 1041-1043, issn 0004-6280Conference Paper

Electron temperature variations and the measurement of nebular abundancesGARNETT, D. R.The Astronomical journal (New York). 1992, Vol 103, Num 4, pp 1330-1337, issn 0004-6256Article

The abundance of sulfur in extragalactic H II regionsGARNETT, D. R.The Astrophysical journal. 1989, Vol 345, Num 1, pp 282-297, issn 0004-637X, 1Article

Observations of [S IV] and the O/S abundance ratio in two halo population planetary nebulaeGARNETT, D. R; LACY, J. H.The Astrophysical journal. 1993, Vol 419, Num 2, pp L93-L96, issn 0004-637X, 2Article

He II emission in extragalactic H II regionsGARNETT, D. R; KENNICUTT, R. C; YOU-HUA CHU et al.The Astrophysical journal. 1991, Vol 373, Num 2, pp 458-464, issn 0004-637X, 7 p., p.1Article

Type Ib supernova 1983 n and 1985 f: oxygen-rich late time spectraGASKELL, C. M; CAPPELLARO, E; DINERSTEIN, H. L et al.The Astrophysical journal. 1986, Vol 306, Num 2, pp L77-L80, issn 0004-637XArticle

HII regions with HeII emissionGARNETT, D. R; KENNICUTT, R. C; YOU-HUA CHU et al.Publications of the Astronomical Society of the Pacific. 1991, Vol 103, Num 666, pp 850-852, issn 0004-6280Conference Paper

The abundances of carbon and nitrogen in I Zw 18DUFOUR, R. J; GARNETT, D. R; SHIELDS, G. A et al.The Astrophysical journal. 1988, Vol 332, Num 2, pp 752-761, issn 0004-637X, 1Article

The composition gradient across M81GARNETT, D. R; SHIELDS, G. A.The Astrophysical journal. 1987, Vol 317, Num 1, pp 82-101, issn 0004-637X, 1Article

Deciphering a Rosetta Stone : the nebula MA 1 in M33GARNETT, D. R; ODEWAHN, S. C; SKILLMAN, E. D et al.The Astronomical journal (New York). 1992, Vol 104, Num 5, pp 1714-1720, issn 0004-6256Article

The early spectral phase of type Ib supernovae: evidence for heliumHARKNESS, R. P; WHEELER, J. C; LEVREAULT, R. M et al.The Astrophysical journal. 1987, Vol 317, Num 1, pp 355-367, issn 0004-637X, 1Article

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