6dFGS gJ002339.6-094848 , the SIMBAD biblio

6dFGS gJ002339.6-094848 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST07:03:14


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Title First 3 Authors
2004ApJS..153..429K viz 656 152 Strong emission line H II galaxies in the sloan digital sky survey. I. Catalog of DR1 objects with oxygen abundances from te measurements. KNIAZEV A.Y., PUSTILNIK S.A., GREBEL E.K., et al.
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.
2009MNRAS.399..683J viz 15       D               1 124640 796 The 6dF galaxy survey: final redshift release (DR3) and southern large-scale structures. JONES D.H., READ M.A., SAUNDERS W., et al.
2013ApJ...765...26S viz 16       D               1 301 11 Dissection of Hα emitters: low-z analogs of z > 4 star-forming galaxies. SHIM H. and CHARY R.-R.
2014MNRAS.442.3565C viz 16       D               3 138 77 The L-σ relation for massive bursts of star formation. CHAVEZ R., TERLEVICH R., TERLEVICH E., et al.
2016MNRAS.463.1144W 16       D               1 131 10 The H II galaxy Hubble diagram strongly favours Rh = ct over ΛCDM. WEI J.-J., WU X.-F. and MELIA F.
2017A&A...599A..71D viz 16       D               1 209270 41 Aperture-free star formation rate of SDSS star-forming galaxies. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.
2017A&A...599A..76M viz 16       D               1 139 4 The L-σ relation for HII galaxies in green. MELNICK J., TELLES E., BORDALO V., et al.
2018AJ....155...17C viz 16       D               2 803 ~ Infrared photometric study of Wolf-Rayet galaxies. CHEN P.S., YANG X.H., LIU J.Y., et al.
2022ApJS..258...29C viz 18       D               2 101251 ~ A Uniformly Selected, Southern-sky 6dF, Optical AGN Catalog. CHEN Y.-P., ZAW I., FARRAR G.R., et al.
2022A&A...666A.186D viz 18       D               1 194358 6 Mass-metallicity and star formation rate in galaxies: A complex relation tuned to stellar age. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.

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