Leonard W. Isberner

activity

20222024

most citedExperimental determination of the dissociative recombination rate coefficient for rotationally-cold CH

^{+}

and its implications for the diffuse cloud chemistry

17 citations · 28 across the 3 of their papers we have counts for

collaborators

3 papers

physics.atom-ph2024

Dissociative recombination of rotationally cold ArH $^{+}$

Ábel Kálosi, Manfred Grieser, Leonard W. Isberner +11

We have experimentally studied dissociative recombination (DR) of electronically and vibrationally relaxed ArH $^{+}$ in its lowest rotational levels, using an electron--ion merged-be…

astro-ph.GA2023★ 11 cited

Dissociative Recombination of Rotationally Cold OH $^{+}$ and Its Implications for the Cosmic Ray Ionization Rate in Diffuse Clouds

Ábel Kálosi, Lisa Gamer, Manfred Grieser +12

Observations of OH $^{+}$ are used to infer the interstellar cosmic ray ionization rate in diffuse atomic clouds, thereby constraining the propagation of cosmic rays through and the s…

astro-ph.GA2022★ 17 cited

Experimental determination of the dissociative recombination rate coefficient for rotationally-cold CH $^{+}$ and its implications for the diffuse cloud chemistry

Daniel Paul, Manfred Grieser, Florian Grussie +13

Observations of CH $^{+}$ are used to trace the physical properties of diffuse clouds, but this requires an accurate understanding of the underlying CH $^{+}$ chemistry. Until this work,…

Dissociative recombination of rotationally cold ArH+

Dissociative Recombination of Rotationally Cold OH+ and Its Implications for the Cosmic Ray Ionization Rate in Diffuse Clouds

Experimental determination of the dissociative recombination rate coefficient for rotationally-cold CH+ and its implications for the diffuse cloud chemistry

Dissociative recombination of rotationally cold ArH $^{+}$

Dissociative Recombination of Rotationally Cold OH $^{+}$ and Its Implications for the Cosmic Ray Ionization Rate in Diffuse Clouds

Experimental determination of the dissociative recombination rate coefficient for rotationally-cold CH $^{+}$ and its implications for the diffuse cloud chemistry