First Resolution of a Main-sequence G star’s Astrosphere Using Chandra
C. M. Lisse(Johns Hopkins University Applied Physics Laboratory), L. Gu(Space Research Organisation Netherlands), K. Dennerl(Max Planck Institute for Extraterrestrial Physics), Elena Provornikova(Johns Hopkins University Applied Physics Laboratory), K. Dialynas(Academy of Athens), P. C. Brandt(Max Planck Society), M. Horanyi(Joint Institute for Laboratory Astrophysics), L. J. Paxton(Johns Hopkins University Applied Physics Laboratory), V. Kharchenko(Center for Astrophysics Harvard & Smithsonian), Y. R. Fernandez(University of Central Florida), E. F. Guinan(Villanova University), M. A. MacGregor(Johns Hopkins University Applied Physics Laboratory), P. C. Frisch(University of Chicago), R. L. McNutt(Johns Hopkins University Applied Physics Laboratory), H. M. Günther(Massachusetts Institute of Technology), R. A. Osten(Space Telescope Science Institute), V. Kashyap(Center for Astrophysics Harvard & Smithsonian), S. J. Wolk(Center for Astrophysics Harvard & Smithsonian), J. L. Linsky(Joint Institute for Laboratory Astrophysics), J. H. Debes(Space Telescope Science Institute), K. G. Kislyakova(University of Vienna), S. Redfield(Wesleyan University), J. D. Slavin(Center for Astrophysics Harvard & Smithsonian), C. H. Chen(Space Telescope Science Institute), Bradford Snios(Center for Astrophysics Harvard & Smithsonian), D. C. Hines(Space Telescope Science Institute), Dimitra Koutroumpa(Centre National de la Recherche Scientifique)
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