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Detection of the hydroperoxyl radical HO2 toward rho Ophiuchi A

B. Parise ; Per Bergman (Institutionen för rymd- och geovetenskap, Onsala rymdobservatorium) ; F. Du
Astronomy and Astrophysics (0004-6361). Vol. 541 (2012), p. L11.
[Artikel, refereegranskad vetenskaplig]

Context. Hydrogen peroxide (HOOH) was recently detected toward ρ Oph A. Subsequent astrochemical modeling that included reactions in the gas phase and on the surface of dust grains was able to explain the observed abundance, and highlighted the importance of grain chemistry in the formation of HOOH as an intermediate product in water formation. This study also predicted that the hydroperoxyl radical HO2, the precursor of HOOH, should be detectable. Aims. We aim at detecting the hydroperoxyl radical HO2 in ρ Oph A. Methods. We used the IRAM 30 m and the APEX telescopes to target the brightest HO2 lines at about 130 and 260 GHz. Results. We detect five lines of HO2 (comprising seven individual molecular transitions). The fractional abundance of HO2 is found to be about 10-10, a value similar to the abundance of HOOH. This observational result is consistent with the prediction of the above mentioned astrochemical model, and thereby validates our current understanding of the water formation on dust grains. Conclusions. This detection, anticipated by a sophisticated gas-grain chemical model, demonstrates that models of grain chemistry have improved tremendously and that grain surface reactions now form a crucial part of the overall astrochemical network.

Nyckelord: astrochemistry, line: identification, ISM: abundances, ISM: molecules, ISM: individual objects: ρ Ophiuchi A



Denna post skapades 2012-05-22. Senast ändrad 2015-06-23.
CPL Pubid: 157885

 

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Institutioner (Chalmers)

Institutionen för rymd- och geovetenskap, Onsala rymdobservatorium (2010-2017)

Ämnesområden

Molekylfysik
Astronomi
Stjärnors bildning och utveckling

Chalmers infrastruktur

Onsala rymdobservatorium