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Detection of extragalactic argonium, ArH+, toward PKS 1830-211

Holger S. P. Müller ; Sebastien Muller (Institutionen för rymd- och geovetenskap, Onsala rymdobservatorium) ; Peter Schilke ; Edwin A. Bergin ; John H. Black (Institutionen för rymd- och geovetenskap, Radioastronomi och astrofysik) ; Maryvonne Gerin ; Dariusz C. Lis ; David A. Neufeld ; Sümeyye Suri
Astronomy and Astrophysics (0004-6361). Vol. 582 (2015), p. 4.
[Artikel, refereegranskad vetenskaplig]

Context. Argonium has recently been detected as a ubiquitous molecule in our Galaxy. Model calculations indicate that its abundance peaks at molecular fractions in the range of 10-4 to 10-3 and that the observed column densities require high values of the cosmic ray ionization rate. Therefore, this molecular cation may serve as an excellent tracer of the very diffuse interstellar medium (ISM), as well as an indicator of the cosmic ray ionization rate. Aims. We attempted to detect ArH+ in extragalactic sources to evaluate its diagnostic power as a tracer of the almost purely atomic ISM in distant galaxies. Methods. We obtained ALMA observations of a foreground galaxy at z = 0.89 in the direction of the lensed blazar PKS 1830−211. Results. Two isotopologs of argonium, 36ArH+ and 38ArH+, were detected in absorption along two different lines of sight toward PKS 1830−211, known as the SW and NE images of the background blazar. The argonium absorption is clearly enhanced on the more diffuse line of sight (NE) compared to other molecular species. The isotopic ratio 36Ar/38Ar is 3.46 ± 0.16 toward the SW image, i.e., significantly lower than the solar value of 5.5. Conclusions. Our results demonstrate the suitability of argonium as a tracer of the almost purely atomic, diffuse ISM in high-redshift sources. The evolution of the isotopic ratio with redshift may help to constrain nucleosynthetic scenarios in the early Universe.

Nyckelord: quasars: absorption lines / galaxies: ISM / galaxies: abundances / nuclear reactions, nucleosynthesis, abundances / astrochemistry / quasars: individual: PKS 1830-211



Denna post skapades 2015-11-13. Senast ändrad 2016-01-08.
CPL Pubid: 225697

 

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