Spectral Energy Distribution and Radio Halo of NGC 253 at Low Radio Frequencies
We present new radio continuum observations of NGC 253 from the Murchison Widefield Array at frequencies between 76 and 227 MHz. We model the broadband radio spectral energy distribution for the total flux density of NGC 253 between 76 MHz and 11 GHz. The spectrum is best described as a sum of a cen...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Other Authors: | |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2017
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Online Access: | http://hdl.handle.net/1721.1/109763 https://orcid.org/0000-0003-3336-9958 https://orcid.org/0000-0002-0086-7363 https://orcid.org/0000-0003-0422-2324 https://orcid.org/0000-0002-4117-570X https://orcid.org/0000-0001-7776-7240 https://orcid.org/0000-0001-7670-7190 https://orcid.org/0000-0001-7130-208X |
Internet
http://hdl.handle.net/1721.1/109763https://orcid.org/0000-0003-3336-9958
https://orcid.org/0000-0002-0086-7363
https://orcid.org/0000-0003-0422-2324
https://orcid.org/0000-0002-4117-570X
https://orcid.org/0000-0001-7776-7240
https://orcid.org/0000-0001-7670-7190
https://orcid.org/0000-0001-7130-208X