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      Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades

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          The PLATO 2.0 mission

          H Rauer, C Catalá, C. Aerts … (2014)
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            Fundamental stellar photometry for standards of spectral type on the revised system of the Yerkes spectral atlas

            W. Morgan, H Johnson (1953)
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              Keck Spectra of Pleiades Brown Dwarf Candidates and a Precise Determination of the Lithium Depletion Edge in the Pleiades

              John R. Stauffer, Greg Schultz, J. Davy Kirkpatrick (1998)
              Article 0 comments Cited 253 times – based on 0 reviews     Review now
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                Author and article information

                Journal
                Title: Monthly Notices of the Royal Astronomical Society
                Publisher: Oxford University Press (OUP)
                ISSN (Print): 0035-8711
                ISSN (Electronic): 1365-2966
                Publication date Created: November 2017
                Publication date Created: November 01 2017
                Publication date Created: August 11 2017
                Publication date Other: November 2017
                Publication date (Print): November 01 2017
                Publication date (Electronic): August 11 2017
                Volume: 471
                Issue: 3
                Pages: 2882-2901
                Affiliations
                [1 ] Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
                [2 ] Institut für Astrophysik, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, D-37077 Göttingen, Germany
                [3 ] Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, D-37077 Göttingen, Germany
                [4 ] Oxford Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Rd, Oxford OX1 3RH, UK
                [5 ] Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium
                [6 ] Department of Astrophysics, IMAPP, Radboud University Nijmegen, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands
                [7 ] Center for High Angular Resolution Astronomy and Department of Physics and Astronomy, Georgia State University, PO Box 5060, Atlanta, GA 30302-410, USA
                [8 ] Institute for Astronomy, University of Hawai‘i, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
                [9 ] Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia
                [10 ] SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043, USA
                [11 ] The CHARA Array of Georgia State University, Mount Wilson Observatory, Mount Wilson, CA 91023, USA
                [12 ] NASA Ames Research Center, Moffett Field, CA 94035, USA
                [13 ] Bay Area Environmental Research Inst., 560 Third St., West Sonoma, CA 95476, USA
                [14 ] Laboratoire AIM, CEA/DRF - CNRS - Univ. Paris Diderot - IRFU/SAp, Centre de Saclay, F-91191 Gif-sur-Yvette Cedex, France
                [15 ] Research School of Astronomy & Astrophysics, Australian National University, Canberra, ACT 2611, Australia
                [16 ] Center for Space Science, NYUAD Institute, New York University Abu Dhabi, PO Box 129188, Abu Dhabi, UAE
                Article
                DOI: 10.1093/mnras/stx1050
                SO-VID: 9f06223c-3f57-42f0-b932-a1725d889d46
                Copyright © © 2017
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