Radio background and IGM heating due to Pop III supernova explosions

Jana, R.; Nath, B.B.; Biermann, P.L.

doi:10.1093/mnras/sty3426

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Radio background and IGM heating due to Pop III supernova explosions

Jana, R., Nath, B., & Biermann, P. (2019). Radio background and IGM heating due to Pop III supernova explosions. mnras, 483(4), 5329-5333. doi:10.1093/mnras/sty3426.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0006-7AA8-4 Version Permalink: https://hdl.handle.net/21.11116/0000-0006-7AA9-3

Genre: Journal Article

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Creators:
Jana, R., Author
Nath, B.B., Author
Biermann, P.L.¹, Author

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1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652

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Free keywords: supernovae: general, cosmic rays, intergalactic medium, dark ages, reionization, first stars, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics

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Dates: Date issued: 2019-03

Publication Status: Issued

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Identifiers: DOI: 10.1093/mnras/sty3426
BibTex Citekey: 2019MNRAS.483.5329J

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Title: mnras

Source Genre: Journal

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Pages: - Volume / Issue: 483 (4) Sequence Number: - Start / End Page: 5329 - 5333 Identifier: -