Do Kepler Superflare Stars Really Include Slowly Rotating Sun-like Stars?—Results Using APO 3.5 m Telescope Spectroscopic Observations and Gaia-DR2 Data

Author(s):: Notsu, Y.; Maehara, H.; Honda, S.; Hawley, S.L.; Davenport, J.R.A.; Namekata, K.; Notsu, S.; Ikuta, K.; Nogami, D.; Shibata, K.

Published: 2019
Publication type: Article / Letter to editor

Date issued: 2019-05-03
Language: English
Is part of: Astrophysical Journal (0004-637X) (2019), Vol. 876, no. 1, p. 58
hdl: 1887/85026
doi: 10.3847/1538-4357/ab14e6
URL: https://ui.adsabs.harvard.edu/abs/2019ApJ...876...58N