activity
19942009
most citedUltraviolet Survey of CO and H_2 in Diffuse Molecular Clouds: The Reflection of Two Photochemistry Regimes in Abundance Relationships

283 citations · 1k across the 17 of their papers we have counts for

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Showing 2003 · astro-phShow all

7 papers · 2 filters

astro-ph2003

Magnesium isotope ratios in Hyades stars

David Yong, David L. Lambert, Carlos Allende Prieto +1

Using classical model atmospheres and an LTE analysis, Mg isotope ratios 24Mg:25Mg:26Mg are measured in 32 Hyades dwarfs covering 4000K < Teff < 5000K. We find no significant trend…

astro-ph2003

Magnesium isotopic abundance ratios in cool stars

David Yong, David L. Lambert, Inese I. Ivans

From high resolution spectra of 61 cool dwarfs and giants, Mg isotopic abundance ratios 24Mg:25Mg:26Mg are derived from spectral synthesis of the MgH A-X lines near 5140A. Our samp…

astro-ph2003

Finding cool subdwarfs using a V-J reduced proper-motion diagram: Stellar parameters for 91 candidates

David Yong, David L. Lambert

We present the results of a search for cool subdwarfs for which our candidates were drawn from a V-J reduced proper-motion diagram constructed by Salim & Gould (2002). Kinematic (U…

astro-ph2003

Fluorine Abundances in the Large Magellanic Cloud and Omega Centauri: Evidence for Neutrino Nucleosynthesis?

K. Cunha, V. V. Smith, D. L. Lambert +1

The behavior of fluorine with metallicity has not yet been probed in any stellar population. In this work, we present the first fluorine abundances measured outside of the Milky Wa…

astro-ph2003

Further Evidence for Chemical Fractionation from Ultraviolet Observations of Carbon Monoxide

S. R. Federman, David L. Lambert, Yaron Sheffer +4

Ultraviolet absorption from interstellar 12CO and 13CO was detected toward rho Oph A and chi Oph. The measurements were obtained at medium resolution with the Goddard High Resoluti…

astro-ph2003

Non-LTE Model Atmospheres for Late-Type Stars II. Restricted NLTE Calculations for a Solar-Like Atmosphere

C. Allende Prieto, I. Hubeny, D. L. Lambert

We test our knowledge of the atomic opacity in the solar UV spectrum. Using the atomic data compiled in Paper I from modern, publicly available, databases, we perform calculations…