activity
20022008
most citeds-Process Abundances in Planetary Nebulae

108 citations · 320 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph2008★ 22 cited

Independent Emission and Absorption Abundances for Planetary Nebulae

Robert Williams, Edward B. Jenkins, Jack A. Baldwin +4

Emission-line abundances have been uncertain for more than a decade due to unexplained discrepancies in the relative intensities of the forbidden lines and weak permitted recombina…

astro-ph2006★ 108 cited

s-Process Abundances in Planetary Nebulae

Brian Sharpee, Yong Zhang, Robert Williams +5

The s-process should occur in all but the lower mass progenitor stars of planetary nebulae, and this should be reflected in the chemical composition of the gas which is expelled to…

astro-ph2006★ 4 cited

Abundances of s-process elements in planetary nebulae: Br, Kr & Xe

Y. Zhang, R. Williams, E. Pellegrini +5

We identify emission lines of post-iron peak elements in very high signal-to-noise spectra of a sample of planetary nebulae. Analysis of lines from ions of Kr and Xe reveals enhanc…

astro-ph2004★ 30 cited

Identification and Characterization of Faint Emission Lines in the Spectrum of the Planetary Nebula IC 418

Brian Sharpee, Jack A. Baldwin, Robert Williams

We present high signal-to-noise echelle spectra of the compact high surface brightness, low ionization planetary nebula IC 418. These reveal 807 emission lines down to intensities…

astro-ph2004★ 47 cited

The Changing Blazhko Effect of XZ Cygni

Aaron LaCluyze, Horace A. Smith, E. -M. Gill +9

New CCD photometry has been obtained for the RR Lyrae variable star XZ Cygni. An analysis of old and new photometry confirms earlier results that XZ Cygni exhibits the Blazhko Effe…

astro-ph2004★ 18 cited

Measurements of the Singly Ionized Oxygen Auroral Doublet Lines 7320,7330ÅUsing High Resolution Sky Spectra

Brian D. Sharpee, Tom G. Slanger, David L. Huestis +1

The wavelengths of the individual [O II] 2s22p3 2Do(5/2) - 2s22p3 2Po(1/2,3/2) 7320Åand [O II] 2s22p3 2Do(3/2) - 2s22p3 2Po(1/2,3/2) 7330Åauroral doublet component lines have been…