LMC & SMC PNe optical spectroscopy. III Virtual Observatory Resource

Authors

1. Vassiliadis E.
2. Dopita M.A.
3. Morgan D.H.
4. Bell J.F.

Published by

CDS

Abstract

We present optical spectroscopy in the range 3300-7400A for a total of 52 planetary nebulae in the Large Magellanic Cloud (LMC) and 18 in the Small Magellanic Cloud (SMC). Together with the object from the first (1991ApJS...75..407M) and second (1991ApJS...76.1085M) papers, we now have accurate emission-line intensities for a total of 147 nebulae in the Magellanic Clouds. This sample contains a large selection of objects of low luminosity, with measurements of line intensities down to ~10% of H{beta}. Brighter objects have line intensities measured down to ~2% of H{beta}. Agreement with other authors is generally very good, especially for lines greater than approximately 10% of H{beta}. Reddening estimates from Balmer line ratios have been determined: unreddened and reddened line intensities are tabulated.

Keywords

1. magellanic-clouds
2. spectroscopy

Bibliographic source Bibcode

1992ApJS...83...87V

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/83/87

IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJS/83/87

Document Object Identifer DOI

doi:10.26093/cds/vizier.20830087

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/83/87
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/83/87
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/83/87

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).