Optical spectra of radio planetary nebulae in the small Magellanic cloud

Article


Payne, J.L., Filipovic, M.D., Crawford, E.J., De Horta, A.Y., White G.L. and H.Stootman, F.H.. 2008. "Optical spectra of radio planetary nebulae in the small Magellanic cloud ." Serbian Astronomical Journal. 2008 (176), pp. 65-70. https://doi.org/10.2298/SAJ0876065P
Article Title

Optical spectra of radio planetary nebulae in the small Magellanic cloud

ERA Journal ID41911
Article CategoryArticle
AuthorsPayne, J.L., Filipovic, M.D., Crawford, E.J., De Horta, A.Y., White G.L. and H.Stootman, F.H.
Journal TitleSerbian Astronomical Journal
Journal Citation2008 (176), pp. 65-70
Number of Pages6
Year2008
PublisherAstronomical Observatory of Belgrade
Place of PublicationSerbia
ISSN1450-698X
Digital Object Identifier (DOI)https://doi.org/10.2298/SAJ0876065P
Web Address (URL)https://doiserbia.nb.rs/Article.aspx?ID=1450-698X0876065P
Abstract

We present preliminary results from spectral observations of four (4) candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4″/2″). Optical PNe and radio candidates are within 2″ and may represent a sub-population of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 M⊙ or greater, supporting the existence of PNe progenitor central stars with masses up to 8 M⊙.

KeywordsIndividual: N9, SMP11; N61; N68; Planetary nebulae
Public Notes

File reproduced in accordance with the copyright policy of the publisher/author.

Page Range65-70
Byline AffiliationsJames Cook University
University of Western Sydney
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