Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-04-29
Astronomy and Astrophysics
Astrophysics
6 pages 8 figures, to be published in Serbian Astronomical Journal
Scientific paper
10.2298/SAJ0876065P
We present preliminary results from spectral observations of four 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 subpopulation of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 MSol or greater, supporting the existence of PNe progenitor central stars with masses up to 8 MSol.
Crawford Evan J.
de Horta Ain Yaci
Filipović Miroslav D.
Payne Jeff L.
Stootman F. H.
No associations
LandOfFree
Optical Spectra of Radio Planetary Nebulae in the Small Magellanic Cloud 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 Optical Spectra of Radio Planetary Nebulae in the Small Magellanic Cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical Spectra of Radio Planetary Nebulae in the Small Magellanic Cloud will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-209394