HS 1214+3801 , the SIMBAD biblio

HS 1214+3801 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST04:12:41


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Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
1995ApJS...98...41P 527 17 The Case low-dispersion northern sky survey. XV. A region in Ursa Major and Canes Venatici. PESCH P., STEPHENSON C.B. and MacCONNELL D.J.
2000A&AS..142..417H viz 101 12 The Hamburg/SAO survey for emission-line galaxies. III. The third list of 81 galaxies. HOPP U., ENGELS D., GREEN R.F., et al.
2004ApJ...602..200I viz 1 82 259 Systematic effects and a new determination of the primordial abundance of 4He and dY/dZ from observations of blue compact galaxies. IZOTOV Y.I. and THUAN T.X.
2006ApJ...646..691F 31 66 Primordial helium abundance: a reanalysis of the Izotov-Thuan spectroscopic sample. FUKUGITA M. and KAWASAKI M.
2006A&A...459...85N viz 15       D               133 302 Gas metallicity diagnostics in star-forming galaxies. NAGAO T., MAIOLINO R. and MARCONI A.
2007ApJ...662...15I viz 15       D               335 213 The primordial abundance of 4He: a self-consistent empirical analysis of systematic effects in a large sample of low-metallicity H II regions. IZOTOV Y.I., THUAN T.X. and STASINSKA G.
2008MNRAS.383..209H 16       D               1 55 112 Precision abundance analysis of bright HII galaxies. HAGELE G.F., DIAZ A.I., TERLEVICH E., et al.
2012MNRAS.424.2316P viz 15       D               1 298 113 `Counterpart' method for abundance determinations in HII regions. PILYUGIN L.S., GREBEL E.K. and MATTSSON L.
2013MNRAS.428.1790W viz 15       D               1 221 14 A blind HI survey in the Ursa Major region. WOLFINGER K., KILBORN V.A., KORIBALSKI B.S., et al.
2015ApJS..217...27A viz 16       D               1 5847 53 A catalog of visually classified galaxies in the local (z ∼ 0.01) universe. ANN H.B., SEO M. and HA D.K.
2016MNRAS.460.1739V viz 16       D               1 615 58 BOND: Bayesian Oxygen and Nitrogen abundance Determinations in giant H II regions using strong and semistrong lines. VALE ASARI N., STASINSKA G., MORISSET C., et al.

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