Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
UW-Oshkosh
Department of Physics and Astronomy, University of Wisconsin Oshkosh
U. Wisconsin-Oshkosh
U. Wisconsin-Oshkoch
University of Wisconsin-Oshkosh
University of Texas, Austin, TX, US
Department of Physics and Astronomy, University of Wisconsin, Oshkosh, 800 Algoma Boulevard, Oshkosh, WI 54901
Department of Physics and Astronomy, University of Wisconsin at Oshkosh, Oshkosh, WI 54901
National Science Foundation, Division of Astronomical Sciences, Arlington, VA 2223; Any opinions, findings, conclusions, and recommendations expressed in this material are those of the authors and do not necessarily reflect the views of the National Science Foundation; Department of Physics and Astronomy, University of Wisconsin, 800 Algoma Boulevard, Oshkosh, WI 54901.
McDonald Observatory; Texas Univ., Austin
Maryland, University, College Park
Department of Physics and Astronomy, University of Wisconsin-Oshkosh, Oshkosh, WI 54901 of Physics and Astronomy, University of Wisconsin-Oshkosh, 800 Algoma Boulevard, Oshkosh, WI 54901
McDonald Observatory, Austin, TX
Department of Physics and Astronomy, University of Wisconsin, 800 Algoma Boulevard, Oshkosh, WI 54901
University of Wisconsin
University of Wisconsin Oshkosh
University of Wisconsin Oshkosh, Oshkosh, WI 54901, USA
University of Texas
U Wisc. Oshkosh
Univ. Wisc. Oshkosh
U Wisc Oshkosh
University of Wisconsin at Oshkosh
NSF, University of Washington-Oshkosh
Department of Physics and Astronomy, University of Wisconsin Oshkosh, 800 Algoma Blvd., Oshkosh, WI 54901, USA
University of Wisconsin Oshkosh and NSF
University Wi
A Comparison between Carbon and Nitrogen Abundances of Bright Giants in the Globular Clusters M13, M10, and NGC 7006
A Spectroscopic Analysis of the Lithium Rich Star K301 in NGC 7789
Abundances in Stars from the Red Giant Branch Tip to the Main Sequence in M71
Abundances in Stars from the Red Giant Branch Tip to the Near Main Sequence in M71: II. Iron Abundance
Abundances in Stars from the Red Giant Branch Tip to the Near the Main Sequence in M71: I. Sample Selection, Observing Strategy and Stellar Parameters
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