2005/10/04 by D. Rosa‐González, Daniel Rosa-Gonzalez
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Dwarf galaxy #Flux (metallurgy) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Milky Way #Physics #Star formation #Supernova #Supernova remnant #astro-ph
paper · pdf · doi:10.1111/j.1365-2966.2005.09663.x
published as Mon.Not.Roy.Astron.Soc.364:1304-1308,2005 · Accepted for publication in MNRAS
arxiv created 2005/10/04 · openalex publication_date 2005/11/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We present the first subarcsecond radio observations of the nearby dwarf starburst galaxy NGC 3077 obtained with the MERLIN interferometer. We have detected two resolved sources which are coincident with the positions of two discrete X-ray sources detected by Chandra. One of the radio sources is associated with a supernova remnant (SNR) and the observed radio flux is consistent with having a non-thermal origin. The age of the SNRs of about 760 yr is between the average age of the SNRs detected in M82 and those detected in the Milky Way and the Large Magellanic Cloud. We use this detection to calculate a star formation rate (SFR) of 0.28 M⊙ yr−1, which is similar to the SFR calculated by using far-infrared and millimetre observations but larger than the SFR given by optical recombination lines corrected for extinction. The other compact radio source detected by MERLIN, which is coincident with the position of an X-ray binary, has the properties of an H ii region with a flux density of about 747 μJy, which corresponds to an ionizing flux of 6.8 × 1050 s−1. A young massive stellar cluster with a mass of ∼2 × 105 M⊙ detected by the Hubble Space Telescope could be responsible for the production of the ionizing flux.