LMC PNe [OIII] 5007Å and Hβ flux (Reid+, 2010)

Details LMC PNe [OIII] 5007Å and Hβ flux (Reid+, 2010) LMC PNe [OIII] 5007Å and Hβ flux (Reid+, 2010)

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..74051349r&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/405/1349. Originally published in: 2010MNRAS.405.1349R

Physics

Magellanic Clouds, Planetary Nebulae, Spectroscopy

Scientific paper

A five night observing run on the Anglo-Australian Telescope (AAT) using 2dF was undertaken in 2004 December to spectroscopically confirm LMC emission candidates as PNe and to eliminate contaminants such as HII regions and emission-line stars.
The observations provided ~4000 spectra. Individual exposure times were mostly 1200s using the 300B grating with a central wavelength of 5852Å and a wavelength range of 3600-8000Å at a dispersion of 4.30Å/pix.
(2 data files).

Affiliated with

Also associated with

No associations

Rating

LMC PNe [OIII] 5007Å and Hβ flux (Reid+, 2010) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with LMC PNe [OIII] 5007Å and Hβ flux (Reid+, 2010), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and LMC PNe [OIII] 5007Å and Hβ flux (Reid+, 2010) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1534050