Astrophys. J., 656, 168-185 (2007/February-2)
The localized chemical pollution in NGC 5253 revisited: results from deep echelle spectrophotometry.
LOPEZ-SANCHEZ A.R., ESTEBAN C., GARCIA-ROJAS J., PEIMBERT M. and RODRIGUEZ M.
Abstract (from CDS):
We present echelle spectrophotometry of the blue compact dwarf galaxy NGC 5253 obtained with the VLT UVES. We have measured the intensities of a large number of permitted and forbidden emission lines in four zones of the central part of the galaxy. We detect faint C II and O II recombination lines, the first time that these are unambiguously detected in a dwarf starburst galaxy. The physical conditions of the ionized gas have been derived using a large number of different line intensity ratios. Chemical abundances of He, N, O, Ne, S, Cl, Ar, and Fe have been determined following standard methods. C++ and O++ abundances have been derived from pure recombination lines and are larger than those obtained from collisionally excited lines (from 0.30 to 0.40 dex for C++ and from 0.19 to 0.28 dex for O++). This result is consistent with a temperature fluctuation parameter (t2) between 0.050 and 0.072. We confirm previous results that indicate the presence of a localized N enrichment in certain zones of NGC 5253 and detect a possible slight He overabundance in the same zones. The enrichment pattern agrees with that expected for the pollution by the ejecta of Wolf-Rayet (W-R) stars. The amount of enriched material needed to produce the observed overabundance is consistent with the mass lost by the number of W-R stars estimated in the starbursts. We discuss the possible origin of the difference between abundances derived from recombination and collisionally excited lines (the so-called abundance discrepancy problem) in H II regions, finding that a recent hypothesis based on the delayed enrichment by SN ejecta inclusions seems not to explain the observed features.
Galaxies: Abundances - galaxies: clusters: individual (NGC 5253) - Galaxies: Kinematics and Dynamics - Galaxies: Starburst
VizieR on-line data:
<Available at CDS (J/ApJ/656/168): table2.dat>
Fig.2: the designation 'A' is not used in SIMBAD: A = KSRWR HII-2, B = KSRWR HII-1, C = KSRWR UV-1, D = KSRWR UV-2.
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