Structure and feedback in 30 Doradus. I. (Pellegrini+, 2010)

Details Structure and feedback in 30 Doradus. I. (Pellegrini+, 2010) Structure and feedback in 30 Doradus. I. (Pellegrini+, 2010)

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..21910160p&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/191/160. Originally published in: 2010ApJS..191..160P

Physics

Interstellar Medium, Spectroscopy

Scientific paper

In 2008 February, we obtained a grid of long-slit spectra of 30 Dor using the RC spectrograph on the 4m Blanco telescope at Cerro Tololo Inter-American Observatory (CTIO). The spectrograph slit was 5 arcmin in length, and was positioned at a total of 37 different locations spanning the nebula (Figure 1(b)). Table 2 lists for each slit position the identifying position number, the R.A. and decl. of the slit center in J2000 coordinates, the P.A., and the total exposure time.
(2 data files).

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