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19942025
most citedC and N Abundances in Stars At the Base of the Red Giant Branch in M5

117 citations · 875 across the 22 of their papers we have counts for

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16 papers · 1 filter

astro-ph2008★ 76 cited

Stellar Population Models and Individual Element Abundances II: Stellar Spectra and Integrated Light Models

H. -c. Lee, G. Worthey, A. Dotter +7

The first paper in this series explored the effects of altering the chemical mixture of the stellar population on an element by element basis on stellar evolutionary tracks and iso…

astro-ph2008★ 70 cited

Deep Mixing and Metallicity: Carbon Depletion in Globular Cluster Giants

Sarah L. Martell, Graeme H. Smith, Michael M. Briley

We present the results of an observational study of the efficiency of deep mixing in globular cluster red giants as a function of stellar metallicity. We determine [C/Fe] abundance…

astro-ph2008★ 20 cited

An Improved Bandstrength Index for the CH G Band of Globular Cluster Giants

Sarah L. Martell, Graeme H. Smith, Michael M. Briley

Spectral indices are useful tools for quantifying the strengths of features in moderate-resolution spectra and relating them to intrinsic stellar parameters. This paper focuses on…

astro-ph2007★ 38 cited

CN Bimodality at Low Metallicity: The Globular Cluster M53

Sarah L. Martell, Graeme H. Smith, Michael M. Briley

We present low resolution UV-blue spectroscopic observations of red giant stars in the globular cluster M53 ([Fe/H]=-1.84), obtained to study primordial abundance variations and de…

astro-ph2007

The New Standard Stellar Population Models (NSSPM) -- The Prologue

Hyun-chul Lee, Guy Worthey, Scott C. Trager +7

We are developing a brand new stellar population models with flexible chemistry (isochrones plus stellar colors and spectra) in order to set a new standard of completeness and exce…

astro-ph2005★ 82 cited

C and N Abundances in Stars At the Base of the Red Giant Branch in M15

Judith G. Cohen, Michael M. Briley, Peter B. Stetson

We present an analysis of a large sample of moderate resolution Keck LRIS spectra of subgiants and stars at the base of the RGB in M15, most within the range 16.5 < V < 19.5 (1.2 <…