UGC 6345 B , the SIMBAD biblio

UGC 6345 B , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:14:18

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1988AJ.....96.1192S 46 32 The far-infrared properties of optically selected emission-line galaxies. SALZER J.J. and MacALPINE G.M.
1989ApJS...70..447S 175 102 Observations of a complete sample of emission-line galaxies. I. CCD imaging and spectroscopy of galaxies in UM lists IV and V. SALZER J.J., MacALPINE G.M. and BOROSON T.A.
1989ApJS...70..479S 148 102 Observations of a complete sample of emission-line galaxies. II. Properties of the UM survey galaxies. SALZER J.J., MacALPINE G.M. and BOROSON T.A.
1991A&A...241..358C 70 43 Environmental properties of violenty star-forming galaxies. CAMPOS-AGUILAR A. and MOLES M.
1991A&AS...91..285T viz 419 345 A spectrophotometric catalogue of HII galaxies. TERLEVICH R., MELNICK J., MASEGOSA J., et al.
1993AJ....106.1784C 85 62 Empirical characterization of blue dwarf galaxies. CAMPOS-AGUILAR A., MOLES M. and MASEGOSA J.
1995AJ....110.1090V 58 64 On the spectroscopic properties of star-forming dwarf galaxies in different environments. VILCHEZ J.M.
1995ApJS...99..427T 36 118 An HI/optical atlas of HII galaxies and their companions. TAYLOR C.L., BRINKS E., GRASHUIS R.M., et al.
1998AJ....116.2746T 83 164 CO emission in low-luminosity, H I-rich galaxies. TAYLOR C.L., KOBULNICKY H.A. and SKILLMAN E.D.
1999Ap.....42..149C 75 3 Study of new sample of candidate blue compact dwarf galaxies. HI observations of 73 objects at Nancay radio telescope. COMTE G., PETROSIAN A.R., OHANIAN G.A., et al.
2000A&A...355...89D viz 259 24 Spectral classification of emission-line galaxies. DESSAUGES-ZAVADSKY M., PINDAO M., MAEDER A., et al.
2000A&A...361...19S 100 24 HI observations of emission-line galaxies. SMOKER J.V., DAVIES R.D., AXON D.J., et al.
2000MNRAS.317..649B 1 11 36 Molecular gas in blue compact dwarf galaxies. BARONE L.T., HEITHAUSEN A., HUETTEMEISTER S., et al.
2001A&A...371..806N 105 42 On faint companions in the close environment of star-forming dwarf galaxies. Possible external star formation triggers? NOESKE K.G., IGLESIAS-PARAMO J., VILCHEZ J.M., et al.
2002AJ....124..191S 144 26 An H I survey of actively star-forming dwarf galaxies. SALZER J.J., ROSENBERG J.L., WEISSTEIN E.W., et al.
2003AJ....126.2774H 70 11 Neutral hydrogen mapping of Virgo cluster blue compact dwarf galaxies. HOFFMAN G.L., BROSCH N., SALPETER E.E., 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.
2006MNRAS.365..454H viz 408 26 The impact of the visibility of the [OIII]λ4363 line on the general properties of HII galaxies in the Local Universe. HOYOS C. and DIAZ A.I.
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.
2011PASJ...63L...1K 24 8 Deep CO observations and the CO-to-H2 conversion factor in DDO 154, a low metallicity dwarf irregular galaxy. KOMUGI S., YASUI C., KOBAYASHI N., et al.
2013ApJ...769...82S viz 15       D               1 326 20 The fueling diagram: linking galaxy molecular-to-atomic gas ratios to interactions and accretion. STARK D.V., KANNAPPAN S.J., WEI L.H., et al.
2013A&A...556A..10M viz 1052       D     X C F     26 23 8 Deep multiband surface photometry on a sample of 24 blue compact galaxies. II. A volume-limited sample of 21 emission line galaxies. MICHEVA G., OESTLIN G., ZACKRISSON E., et al.
2016MNRAS.460.1739V viz 16       D               2 615 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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