Extragalactic H3O+: Some Consequences
Floris van der Tak (SRON Groningen, NL), Susanne Aalto (Onsala, S),, Rowin Meijerink (Berkeley, USA)
TL;DR
This paper explores the implications of detecting extragalactic H3O+ in M82, focusing on gas location, energetic radiation origins, and star formation feedback effects on cosmic rays.
Contribution
It presents new insights into the role of H3O+ in understanding galaxy environments and star formation feedback mechanisms.
Findings
H3O+ detected in M82 provides clues about gas distribution.
Star formation influences cosmic ray flux in galaxies.
Implications for energetic radiation sources in M82.
Abstract
We discuss some implications of our recent detection of extragalactic H3O+: the location of the gas in M82, the origin of energetic radiation in M82, and the possible feedback effects of star formation on the cosmic ray flux in galaxies.
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