div class=ts-pagebutton class=gotoPage data-page=1Page 1button div class=ts-imagea href=https:reader042vdocumentspubreader042viewer20220408195e66a5d6020f7e0e983d423chtml5page1jpg target=_blank img data-url=onetouch-40-scanned-braatenstatphysschroeder7bpdf-2012-01-18-notice-thathtmlpage=1 data-page=1 class=ts-thumb lazyload alt=Page 1: OneTouch 40 Scanned Documentsbraatenstatphysschroeder7Bpdf · 2012-01-18 · Notice that a white dwarf star with a larger mass has a smaller equilibrium radius This does make loading=lazy src=data:imagegifbase64iVBORw0KGgoAAAANSUhEUgAAAAIAAAACCAQAAADYv8WvAAAAD0lEQVR42mP8X8AwAgiABKBAv+vAXklAAAAAElFTkSuQmCC data-src=https:reader042vdocumentspubreader042viewer20220408195e66a5d6020f7e0e983d423chtml5thumbnails1jpg width=140 height=200 adivdivdiv class=ts-pagebutton class=gotoPage data-page=2Page 2button div class=ts-imagea href=https:reader042vdocumentspubreader042viewer20220408195e66a5d6020f7e0e983d423chtml5page2jpg target=_blank img 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a white dwarf star with a larger mass has a smaller equilibrium radius This does make loading=lazy src=data:imagegifbase64iVBORw0KGgoAAAANSUhEUgAAAAIAAAACCAQAAADYv8WvAAAAD0lEQVR42mP8X8AwAgiABKBAv+vAXklAAAAAElFTkSuQmCC data-src=https:reader042vdocumentspubreader042viewer20220408195e66a5d6020f7e0e983d423chtml5thumbnails3jpg width=140 height=200 adivdivdiv class=ts-pagebutton class=gotoPage data-page=4Page 4button div class=ts-imagea href=https:reader042vdocumentspubreader042viewer20220408195e66a5d6020f7e0e983d423chtml5page4jpg target=_blank img data-url=onetouch-40-scanned-braatenstatphysschroeder7bpdf-2012-01-18-notice-thathtmlpage=4 data-page=4 class=ts-thumb lazyload alt=Page 4: OneTouch 40 Scanned Documentsbraatenstatphysschroeder7Bpdf · 2012-01-18 · Notice that a white dwarf star with a larger mass has a smaller equilibrium radius This does make loading=lazy src=data:imagegifbase64iVBORw0KGgoAAAANSUhEUgAAAAIAAAACCAQAAADYv8WvAAAAD0lEQVR42mP8X8AwAgiABKBAv+vAXklAAAAAElFTkSuQmCC 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src=data:imagegifbase64iVBORw0KGgoAAAANSUhEUgAAAAIAAAACCAQAAADYv8WvAAAAD0lEQVR42mP8X8AwAgiABKBAv+vAXklAAAAAElFTkSuQmCC data-src=https:reader042vdocumentspubreader042viewer20220408195e66a5d6020f7e0e983d423chtml5thumbnails8jpg width=140 height=200 adivdivdiv class=ts-pagebutton class=gotoPage data-page=9Page 9button div class=ts-imagea href=https:reader042vdocumentspubreader042viewer20220408195e66a5d6020f7e0e983d423chtml5page9jpg target=_blank img data-url=onetouch-40-scanned-braatenstatphysschroeder7bpdf-2012-01-18-notice-thathtmlpage=9 data-page=9 class=ts-thumb lazyload alt=Page 9: OneTouch 40 Scanned Documentsbraatenstatphysschroeder7Bpdf · 2012-01-18 · Notice that a white dwarf star with a larger mass has a smaller equilibrium radius This does make loading=lazy src=data:imagegifbase64iVBORw0KGgoAAAANSUhEUgAAAAIAAAACCAQAAADYv8WvAAAAD0lEQVR42mP8X8AwAgiABKBAv+vAXklAAAAAElFTkSuQmCC data-src=https:reader042vdocumentspubreader042viewer20220408195e66a5d6020f7e0e983d423chtml5thumbnails9jpg 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