Hornstein / Pasadena / New York / Riverside / Kamuela / Berlin / Scoville / Los Angeles / Toronto / Honolulu / Murray / /
Company
Wilson / Wright S. A. / /
Country
United States / Canada / /
Currency
USD / / /
Facility
University of California Riverside / University of California Los Angeles / Dam et al. / University Ave. / University of Hawaii / University of Toronto / Dunlap Institute / Portola Plaza / California Institute of Technology / Galactic Center / University of California / W. M. Keck Observatory / /
IndustryTerm
e-prints / by-product / pure gas cloud model / binary star merger product / pure gas model / earth mass gas cloud / extinction law / pure disrupting gas cloud scenario / putative stellar merger products / hot gas / merger product / adaptive optics technologies / structured gas streams / gas cloud model / pure gas cloud / orbital solutions / face-on systems / binary systems / gas cloud / /
Organization
California Institute of Technology / University of California / Galactic Center / National Science Foundation / Preston / W. M. Keck Foundation / Institute for Astronomy / Leichtman Family Foundation / African Union / Division of Physics / Mathematics / and Astronomy / University of Hawaii / University of California Los Angeles / National Aeronautics and Space Administration / University of Toronto / University of California Riverside / Dunlap Institute for Astronomy and Astrophysics / /
Person
binary star / Gerry Neugebauer / /
Position
Astronomer / rt / tidal radius rt / model / natural model for G2 / /
Accepted by ApJ Letters, 2014 October 14 Preprint typeset using LATEX style emulateapj v[removed]DETECTION OF GALACTIC CENTER SOURCE G2 AT 3.8 MICRONS DURING PERIAPSE PASSAGE G. Witzel1 , A. M. Ghez1 , M. R. Morris1 , B.