Dissociative recombination of rotationally cold H3

By B. McCall, A. Huneycutt, R. Saykally, N. Djurić, G. Dunn, J. Semaniak, O. Novotný, A. Al-Khalili, A. Ehlerding, F. Hellberg and 6 more. 2004

134 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/5234f929ddbd89c5f9ddaa16f16ad402adc44833

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. S. Glover
2. Ralf Klessen
3. Christoph Federrath
4. N. Indriolo
5. B. McCall
6. T. Snow
7. T. Geballe
8. P. Hennebelle

In Atomic and Molecular Physics, and Optics

1. S. Glover
2. Ralf Klessen
3. N. Indriolo
4. B. McCall
5. T. Snow
6. T. Oka

In Spectroscopy

1. Ralf Klessen
2. S. Glover
3. N. Indriolo
4. T. Geballe
5. A. Burgasser

Citations in the corpus

• Physical Processes in the Interstellar Medium (2014, background): “(17) Since all of the column densities on the right-hand side of this expression can be measured observationally (see e.g. Savage et al., 1977; Cardelli et al., 1996; McCall et al., 2002), and kdr can be measured experimentally (McCall et al., 2004), we can use this expression to constrain ζH2 .”
• Hot and Diffuse Clouds near the Galactic Center Probed by Metastable H3+ (2005, methodology): “Finally, note that discussions of the cloud dimension L and the ionization rate ζ in this section 4.4 are based on the dissociative recombination rate constant ke reported by McCall et al. (2003, 2004).”
• INVESTIGATING THE COSMIC-RAY IONIZATION RATE IN THE GALACTIC DIFFUSE INTERSTELLAR MEDIUM THROUGH OBSERVATIONS OF H+3 (2011, methodology): “The H+3 -electron recombination rate coefficient has now been measured in multiple laboratory experiments (e.g., McCall et al. 2004; Kreckel et al. 2005, 2010) with consistent results and is presented in Table 3.”
• Modelling CO formation in the turbulent interstellar medium (2009, unknown): “…(1976a,b), 67: Petuchowski et al. (1989), 68: Federer et al. (1984a,b), 69: Peart & Hayton (1994) 70: Fit by Woodall et al. (2007) to data from McCall et al. (2004), 71: Takagi, Kosugi, & Le Dourneuf (1991), 72: Larson et al. (1998), 73: Mitchell (1990), 74: Guberman (1995), 75: Rosén et al.…”
• Diffuse Atomic and Molecular Clouds (2006, background): “A low recombination rate coefficient seems to be ruled out by recent storage-ring measurements at low temperature (McCall et al. 2004, Kreckel et al. 2005) and supporting theoretical calculations (Kokoouline & Greene 2003).”