2010/01/01 by I. S. Bojicic, I.S. Bojicic, M.D. Filipovic +3
Physics and Astronomy · #Angular diameter #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Emission nebula #Galaxies: Formation, Evolution, Phenomena #Large Magellanic Cloud #Nebula #Planetary nebula #Small Magellanic Cloud #astro-ph.SR
paper · pdf · doi:10.2298/saj1081063b
accepted for publication in Serbian Astronomical Journal
openalex publication_date 2010/01/01 · arxiv created 2010/10/22 · arxiv updated 2015/05/20 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
In this paper we report a new radio-continuum detection of an extragalactic planetary nebula (PN): SMC SMP 24. We show the radio-continuum image of this PN and present the measured radio data. The newly reduced radio observations are consistent with the multi-wavelength data and derived parameters found in the literature. SMC SMP 24 appears to be a young and compact PN, optically thick at frequencies below 2 GHz.