activity
20032015
most citedParent Stars of Extrasolar Planets VII: New Abundance Analyses of 30 Systems

140 citations · 225 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2015★ 21 cited

Quantum Calculation of Inelastic CO Collisions with H. III. Rate Coefficients for Ro-vibrational Transitions

L. Song, N. Balakrishnan, K. M. Walker +5

We present calculated rate coefficients for ro-vibrational transitions of CO in collisions with H atoms for a gas temperature range of 10 K 3000 K, based on the recen…

astro-ph.GA2015

Quantum Calculation of Inelastic CO Collisions with H. II. Pure Rotational Quenching of High Rotational Levels

Kyle M. Walker, L. Song, B. H. Yang +5

Carbon monoxide is a simple molecule present in many astrophysical environments, and collisional excitation rate coefficients due to the dominant collision partners are necessary t…

astro-ph.SR2015★ 16 cited

Collisional quenching of highly rotationally excited HF

Benhui Yang, K. M. Walker, R. C. Forrey +2

Collisional excitation rate coefficients play an important role in the dynamics of energy transfer in the interstellar medium. In particular, accurate rotational excitation rates a…

astro-ph.GA2014★ 40 cited

On the Validity of Collider-Mass Scaling for Molecular Rotational Excitation

Kyle M. Walker, B. H. Yang, P. C. Stancil +2

Rate coefficients for collisional processes such as rotational and vibrational excitation are essential inputs in many astrophysical models. When rate coefficients are unknown, the…

astro-ph.GA2009★ 8 cited

Rubidium in the Interstellar Medium

Kyle M. Walker, S. R. Federman, David C. Knauth +1

We present observations of interstellar rubidium toward o Per, zeta Per, AE Aur, HD 147889, chi Oph, zeta Oph, and 20 Aql. Theory suggests that stable 85Rb and long-lived 87Rb are…

astro-ph2003★ 140 cited

Parent Stars of Extrasolar Planets VII: New Abundance Analyses of 30 Systems

Chris Laws, Guillermo Gonzalez, Kyle M. Walker +4

The results of new spectroscopic analyses of 30 stars with giant planet and/or brown dwarf companions are presented. Values for Teff and [Fe/H] are used in conjunction with Hipparc…