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      Asteroseismic masses of retired planet-hosting A-stars using SONG

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          Detection of possible p-mode oscillations on Procyon

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            Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

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              A New Planet around an M Dwarf: Revealing a Correlation between Exoplanets and Stellar Mass

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                Author and article information

                Journal
                Monthly Notices of the Royal Astronomical Society
                Oxford University Press (OUP)
                0035-8711
                1365-2966
                December 2017
                December 21 2017
                September 06 2017
                December 2017
                December 21 2017
                September 06 2017
                : 472
                : 4
                : 4110-4116
                Affiliations
                [1 ] School of Physics, University of New South Wales, NSW 2052, Australia
                [2 ] Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia
                [3 ] Department of Physics and Astronomy, Stellar Astrophysics Centre, Aarhus University, DK-8000 Aarhus C, Denmark
                [4 ] Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
                [5 ] SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043, USA
                [6 ] Department of Astronomy, Cornell University, Ithaca, NY 14850, USA
                [7 ] Mount Stromlo Observatory, Research School of Astronomy & Astrophysics, The Australian National University, ACT 2611, Australia
                [8 ] Instituto de Astrof sica de Canarias, E-38200 La Laguna, Tenerife, Spain
                Article
                10.1093/mnras/stx2295
                177e6e17-b12f-4dde-8fec-57197ba70919
                © 2017
                History

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