div class=trans-pagebuttonPage 1button div class=trans-image a href=https:reader043fdocumentsusreader043viewer20220413025e132be423bb7e67666d3abehtml5page1jpg target=_blank amp-img class=trans-thumb alt=Page 1: cascacacascacawp-contentuploads201409CAS85_1994_Decpdf · helium persists at low effective temperatures In particular no white dwarf star with a helium-to-hydrogen ratio src=https:reader043fdocumentsusreader043viewer20220413025e132be423bb7e67666d3abehtml5thumbnails1jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=trans-pagebuttonPage 2button div class=trans-image a href=https:reader043fdocumentsusreader043viewer20220413025e132be423bb7e67666d3abehtml5page2jpg target=_blank amp-img class=trans-thumb alt=Page 2: cascacacascacawp-contentuploads201409CAS85_1994_Decpdf · helium persists at low effective temperatures In particular no white dwarf star with a helium-to-hydrogen ratio src=https:reader043fdocumentsusreader043viewer20220413025e132be423bb7e67666d3abehtml5thumbnails2jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=trans-pagebuttonPage 3button div class=trans-image a href=https:reader043fdocumentsusreader043viewer20220413025e132be423bb7e67666d3abehtml5page3jpg target=_blank amp-img class=trans-thumb alt=Page 3: cascacacascacawp-contentuploads201409CAS85_1994_Decpdf · helium persists at low effective temperatures In particular no white dwarf star with a helium-to-hydrogen ratio src=https:reader043fdocumentsusreader043viewer20220413025e132be423bb7e67666d3abehtml5thumbnails3jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=trans-pagebuttonPage 4button div class=trans-image a href=https:reader043fdocumentsusreader043viewer20220413025e132be423bb7e67666d3abehtml5page4jpg target=_blank amp-img class=trans-thumb alt=Page 4: cascacacascacawp-contentuploads201409CAS85_1994_Decpdf · helium persists at low effective temperatures In particular no white dwarf star with a helium-to-hydrogen ratio...