Magellanic Cloud Planetary Nebulae

Home Observations Images Analysis Papers

Catalog of LMC PNe spectra

The 1-D flux (y axis) is in ergs/sec/cm2/angstrom. The wavelength (x axis) is in angstroms. The left part of the spectra are from the G430M data, and the right part are from the G750M data -- note that they are scaled differently in y (flux). The x axis (wavelength) is scaled the same for all objects. Spectra for individual objects are available via the LMC flux page.

Maintained by the MCPN Project Team, with acknowledgements. Some content is restricted (*) until publication. Send comments to Copyright 2001 The Association of Universities for Research in Astronomy, Inc. All Rights Reserved.