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Modelling mid-Z element atmospheres for strongly magnetized neutron stars
Authors:Kaya Mori   Wynn C. G. Ho
Affiliation:Department of Astronomy and Astrophysics, University of Toronto, 50 St George Street, Toronto, Ontario, Canada M5S 3H4;Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St George Street, Toronto, Ontario, Canada M5S 3H8;Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA;Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
Abstract:
Keywords:atomic processes    magnetic fields    stars: atmospheres    stars: neutron
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