2007
DOI: 10.1086/510112
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The Localized Chemical Pollution in NGC 5253 Revisited: Results from Deep Echelle Spectrophotometry

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Cited by 143 publications
(224 citation statements)
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“…To obtain gas mass, we need a gas-to-dust ratio (GTD). Scaled as the oxygen abundance of NGC 5253, 0.2-0.3 solar 13,14 , GTD~650, within the range 340-1200 inferred for the Magellanic clouds 15,16,17 . The observed dust mass is five times larger than the ~3000 M ¤ of dust expected for a 2 x 10 6 M ¤ gas cloud at GTD = 650.…”
mentioning
confidence: 71%
See 1 more Smart Citation
“…To obtain gas mass, we need a gas-to-dust ratio (GTD). Scaled as the oxygen abundance of NGC 5253, 0.2-0.3 solar 13,14 , GTD~650, within the range 340-1200 inferred for the Magellanic clouds 15,16,17 . The observed dust mass is five times larger than the ~3000 M ¤ of dust expected for a 2 x 10 6 M ¤ gas cloud at GTD = 650.…”
mentioning
confidence: 71%
“…53 3) The cluster must be old enough to have Wolf-Rayet (WR) stars, which would explain the WR spectral signatures 13,14,50,51,54,55 . 4) The cluster must have mass less than the virial mass of 1.8 x 10 6 M ¤ , which is also the maximum mass allowed by the [SIV] and Brackett α linewidths 56,57 .…”
Section: Methodsmentioning
confidence: 99%
“…We calculated the N/O and Ne/O abundance ratios assuming that N/O = N + /O + and Ne/O = Ne ++ /O ++ , based on the similarity of the ionization potentials of the ions involved (Peimbert & Costero 1969). This ICF scheme has been used in previous work (e.g., López-Sánchez et al 2007;Hägele et al 2008;Bresolin et al 2009) and is a good approximation for high ionization degree objects. In our spectra, neon is seen via the [NeIII] emission line at 3869 Å.…”
Section: )mentioning
confidence: 99%
“…Another remarkable feature of the starburst region in NGC 5253 is the presence of nitrogen-enriched (by a factor of 2-3) nebular material (Walsh & Roy 1987;Kobulnicky et al 1997;López-Sánchez et al 2007). MonrealIbero et al (2010) have mapped the area of nitrogen enrichment and find it peaks in the giant H ii region, which contains the two nuclear star clusters, and extends up to distances of 3 .3 (50 pc).…”
Section: Introductionmentioning
confidence: 99%