Showing 1–20 of 22 results
/ Date/ Name
Aug 4, 2015Ring Nebulae: Tracers of the CNO NucleosynthesisFeb 3, 2017Carbon and oxygen in HII regions of the Magellanic Clouds: abundance discrepancy and chemical evolutionJan 16, 2012Exploring the effects of high-velocity flows in abundance determinations in H II regions. Bidimensional spectroscopy of HH 204 in the Orion NebulaFeb 25, 2014The Trace of the CNO Cycle in the Ring Nebula NGC6888May 25, 2016The chemical composition of Galactic ring nebulae around massive starsMar 12, 2010Small-spatial scale variations of nebular properties and the abundance discrepancy in three Galactic HII regionsDec 16, 2008Properties of the ionized gas in HH202. I: Results from integral field spectroscopy with PMASJan 27, 2009Properties of the ionized gas in HH202. II: Results from echelle spectrophotometry with UVESJun 18, 2011Integral field spectroscopy of selected areas of the Bright Bar and Orion-S cloud in the Orion NebulaJun 16, 2021Photoionized Herbig-Haro objects in the Orion Nebula through deep high-spectral resolution spectroscopy II: HH204Jun 30, 2015A Consistent Spectral Model of WR 136 and its Associated Bubble NGC 6888Feb 21, 2008M1-78: a nitrogen-rich Galactic compact HII region beyond the Perseus armSep 6, 2013Analysis of chemical abundances in planetary nebulae with [WC] central stars. II. Chemical abundances and the abundance discrepancy factorMay 2, 2012Ionized gas diagnostics from protoplanetary discs in the Orion Nebula and the abundance discrepancy problemOct 14, 2013Deep high spectral resolution spectroscopy and chemical composition of ionized nebulaeApr 25, 2013NGC 2579 and the carbon and oxygen abundance gradients beyond the solar circleMay 27, 2016Protoplanetary disks in the hostile environment of CarinaMay 15, 2009Keck HIRES Spectroscopy of Extragalactic HII Regions: C and O Abundances from Recombination LinesJun 16, 2014Carbon and oxygen abundances from recombination lines in low-metallicity star-forming galaxies. Implications for chemical evolutionJan 6, 2021Photoionized Herbig-Haro objects in the Orion Nebula through deep high-spectral resolution spectroscopy I: HH529II and III