div class=ts-pagebuttonPage 1button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page1jpg target=_blank amp-img class=ts-thumb alt=Page 1: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails1jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 2button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page2jpg target=_blank amp-img class=ts-thumb alt=Page 2: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails2jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 3button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page3jpg target=_blank amp-img class=ts-thumb alt=Page 3: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails3jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 4button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page4jpg target=_blank amp-img class=ts-thumb alt=Page 4: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails4jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 5button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page5jpg target=_blank amp-img class=ts-thumb alt=Page 5: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails5jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 6button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page6jpg target=_blank amp-img class=ts-thumb alt=Page 6: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails6jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 7button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page7jpg target=_blank amp-img class=ts-thumb alt=Page 7: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails7jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 8button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page8jpg target=_blank amp-img class=ts-thumb alt=Page 8: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails8jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 9button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page9jpg target=_blank amp-img class=ts-thumb alt=Page 9: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails9jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 10button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page10jpg target=_blank amp-img class=ts-thumb alt=Page 10: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails10jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 11button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page11jpg target=_blank amp-img class=ts-thumb alt=Page 11: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails11jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 12button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page12jpg target=_blank amp-img class=ts-thumb alt=Page 12: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails12jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 13button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page13jpg target=_blank amp-img class=ts-thumb alt=Page 13: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails13jpg width=142 height=106 layout=responsive amp-imga divdivdiv class=ts-pagebuttonPage 14button div class=ts-image a href=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5page14jpg target=_blank amp-img class=ts-thumb alt=Page 14: · 40 EMISSIVITY Fig 2 - La nostra galassia la Via Lattea come osservata tramite onde radio a 408 MHz emesse da atomi di idro- geno da ESC Garching Germania 1988 Il puntino src=https:reader042vdocumentsusreader042viewer20220411035f0328207e708231d407d1dchtml5thumbnails14jpg width=142 height=106 layout=responsive amp-imga divdiv