Emission-line-object survey in the LMC with the WFI: new faint planetary nebulae.

Details Emission-line-object survey in the LMC with the WFI: new faint planetary nebulae. Emission-line-object survey in the LMC with the WFI: new faint planetary nebulae.

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999msngr..97...29l&link_type=abstract

The Messenger, vol. 97, p. 29-31

Physics

2

Magellanic Clouds: Planetary Nebulae, Magellanic Clouds: H Ii Regions, Magellanic Clouds: Emission-Line Objects, Magellanic Clouds: Be Stars

Scientific paper

The authors' goal is a large survey (10 square degrees in total) of two regions in the SMC and the LMC, to identify new fainter emission-line objects (as PNe, H II regions, Be stars, symbiotic stars, young stars, etc.). They concentrate their efforts mostly on PNe and H II regions. The new candidates allow to derive accurately the full PNe luminosity function in the Magellanic Clouds (MCs), which is still poorly known for faint objects.

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