Spectroscopy of 12 [WC] planetary nebulae (Garcia-Rojas+, 2012)

Garcia-Rojas, J.; Pena, M.; Morisset, C.; Mesa-Delgado, A.; Ruiz, M. T.
Referencia bibliográfica

VizieR On-line Data Catalog: J/A+A/538/A54. Originally published in: 2012A&A...538A..54G

Fecha de publicación:
4
2012
Número de autores
5
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
We acquired spectra at Las Campanas Observatory with the 6.5-m telescope and the Magellan Inamori Kyocera (MIKE) spectrograph, covering a wavelength range from 3350Å to 9400Å on September 2009 and June 2010. The spectra were exposed deep enough to detect, with signal-to-noise ratio higher than three, the weak optical recombination lines (ORLs) of OII, CII, and other species. We detect and identify about 2980 emission lines, which, to date, is the most complete set of spectrophotometric data published for this type of objects. From our deep data, numerous diagnostic line ratios for Te and ne are determined from collisionally excited lines (CELs), ORLs, and continuum measurements (HI Paschen continuum in particular). (3 data files).