LEDA 2678872 , the SIMBAD biblio

LEDA 2678872 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.10CEST10:13:15


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Bibcode/DOI Score in Title|Abstract|
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in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2003A&A...412...45P viz 15       D               1 956205 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
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.
2008A&A...485..657B viz 15       D               578 188 Galaxies with Wolf-Rayet signatures in the low-redshift Universe. A survey using the Sloan Digital Sky Survey. BRINCHMANN J., KUNTH D. and DURRET F.
2010MNRAS.406.1238E 15       D               1 122 44 When are extremely metal-deficient galaxies extremely metal deficient ? EKTA B. and CHENGALUR J.N.
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..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               1 803 ~ Infrared photometric study of Wolf-Rayet galaxies. CHEN P.S., YANG X.H., LIU J.Y., et al.
2020MNRAS.494.1784A viz 17       D               1 47437 9 Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 Mpc. ASMUS D., GREENWELL C.L., GANDHI P., et al.

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