Gemini Spectroscopy of Galactic Bulge Sources 3
PDF hosted at the Radboud Repository of the Radboud University Nijmegen The following full text is a preprint version which may differ from the publisher's version. For additional information about this publication click this link. http://hdl.handle.net/2066/141154 Please be advised that this information was generated on 2021-09-24 and may be subject to change. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 12 January 2015 (MN LATEX style file v2.2) Gemini Spectroscopy of Galactic Bulge Sources: A Population of Hidden Accreting Binaries Revealed?⋆ Jianfeng Wu,1† P. G. Jonker,2,1,3 M. A. P. Torres,2,3 C. T. Britt,4,5,9 C. B. Johnson,4,8 R. I. Hynes,4,8 S. Greiss,6 D. T. H. Steeghs,6,1 T. J. Maccarone,5 C. O. Heinke,7,8 T. Wevers3 1Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 2SRON, Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, The Netherlands 3Department of Astrophysics/IMAPP, Radboud University, Heyendaalseweg 135, 6525 AJ, Nijmegen, The Netherlands 4Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803-4001, USA 5Department of Physics, Texas Tech University, Box 41051, Lubbock TX, 79409-1051, USA 6Department of Physics, University of Warwick, Coventry, CV4 7AL, UK 7Department of Physics, University of Alberta, CCIS 4-183, Edmonton, AB T6G 2E1, Canada 8Max Planck Institute for Radio Astronomy, Auf dem Hugel 69, 53121 Bonn, Germany 9Visiting astronomer, Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which are operated by the Association of Universities for Research in Astronomy, under contract with the National Science Foundation.
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