activity
19972006
most citedThe Chemical Compositions of Galactic Disk F and G Dwarfs

775 citations · 959 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2006★ 50 cited

New Precision Orbits of Bright Double-Lined Spectroscopic Binaries. I: RR Lyncis, 12 Bootis, and HR 6169

Jocelyn Tomkin, Francis C. Fekel

Radial velocities from the 2.1 m telescope at McDonald Observatory supplemented with radial velocities from the coude' feed telescope at KPNO provide new precise orbits for the dou…

astro-ph2002★ 1 cited

Orbits of Hyades Multiple-Lined Spectroscopic Binaries. Paper 2: The Double-Lined System HD 27149

Jocelyn Tomkin

A new determination of the orbit of the Hyades double-lined spectroscopic binary HD 27149 is presented. The well-defined orbit provides the spectroscopic basis for an extremely acc…

astro-ph2002★ 775 cited

The Chemical Compositions of Galactic Disk F and G Dwarfs

Bacham E. Reddy, Jocelyn Tomkin, David L. Lambert +1

Photospheric abundances are presented for 27 elements from carbon to europium in 181 F-G dwarfs from a differential LTE analysis of high-resolution and high signal-to-noise spectra…

astro-ph1999★ 43 cited

The 1995-1996 Decline of R Coronae Borealis - High Resolution Optical Spectroscopy

N. Kameswara Rao, David L. Lambert, Mark T. Adams +10

A set of high-resolution optical spectra of RCrB acquired before, during, and after its 1995-1996 decline is discussed. All of the components reported from earlier declines are see…

astro-ph1999★ 86 cited

Rubidium in Metal-Deficient Disk and Halo Stars

Jocelyn Tomkin, David L. Lambert

We report the first extensive study of stellar Rb abundances. High-resolution spectra have been used to determine, or set upper limits on, the abundances of this heavy element and…

astro-ph1997★ 4 cited

The rise and fall of the NaMgAl stars

Jocelyn Tomkin, Bengt Edvardsson, David L. Lambert +1

We have made new abundance determinations for a sample of NaMgAl stars. These stars, which are a subgroup of the nearby metal-rich field F and G disk dwarfs, were first identified…