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</o:shapelayout></xml><![endif]--></head><body lang=SL link=blue vlink=purple><div class=WordSection1><p class=MsoNormal><o:p> </o:p></p><p class=MsoNormal>Vabimo vas na 7. predavanje iz sklopa "Kolokviji na IJS" v letu 2014/15, ki bo <strong><span style='color:red'>v sredo, 19. novembra 2014, ob 13. uri </span></strong><span style='color:red'>v Veliki predavalnici Instituta »Jožef Stefan«</span> na Jamovi cesti 39 v Ljubljani. Napovednik predavanja najdete tudi na naslovu <a href="http://www.ijs.si/ijsw/Koledar_prireditev">http://www.ijs.si/ijsw/Koledar_prireditev</a>, posnetke preteklih predavanj<span style='color:blue'> </span>pa na <a href="http://videolectures.net/kolokviji_ijs">http://videolectures.net/kolokviji_ijs</a>. <o:p></o:p></p><p class=MsoNormal style='margin-bottom:12.0pt'>~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~<o:p></o:p></p><p class=MsoNormal><b><span lang=EN-US style='mso-fareast-language:ZH-CN'>prof. dr. Tomaž Zwitter<o:p></o:p></span></b></p><p class=MsoNormal><i><span lang=EN-US style='mso-fareast-language:ZH-CN'>Fakulteta za matematiko in fiziko, Univerza v Ljubljani <o:p></o:p></span></i></p><p class=MsoNormal><b><span style='font-size:14.0pt'><o:p> </o:p></span></b></p><p class=MsoNormal align=center style='text-align:center'><b><span lang=EN-US style='font-size:14.0pt'>Medzvezdna snov<o:p></o:p></span></b></p><p class=MsoNormal style='text-align:justify'><span style='font-size:11.0pt;font-family:"Arial","sans-serif"'><o:p> </o:p></span></p><p class=MsoNormal style='text-align:justify'><span lang=EN-US>Prostor med zvezdami ni povsem prazen. V vsakem kubičnem centimetru je pogosto le nekaj deset atomov. To ni veliko, pravzaprav je to redkeje od najboljšega vakuuma, ki ga znamo narediti v laboratoriju. Tako gostoto delcev bi dobili, če bi zrak v kabini vašega avtomobila razporedili po celotni prostornini Zemljine atmosfere. Vendar je vesolje ogromno, zato se v okolici diska naše Galaksije nabere zelo veliko prašnih delcev, atomov in preprostih molekul ter – vse tako kaže – tudi precej zapletenih organskih makromolekul. Žal ne vemo, natanko katere so te molekule. V naši skupini smo se zato lotili alternativnega pristopa in iz opazovanj velikih spektroskopskih pregledov neba skušamo določiti prostorsko porazdelitev teh delcev. Ta nam lahko nekaj pove o njihovih fizikalnih lastnostih, kot je električni naboj ali masa, hkrati pa govori tudi o burnih dogodkih v preteklosti, kot so eksplozije supernov v naši okolici. Morda lahko razloži celo, zakaj v naši relativno stari Galaksiji še vedno ni zmanjkalo plina za nastajanje novih zvezd.</span><b><span lang=ES><o:p></o:p></span></b></p><p class=MsoNormal style='text-align:justify'><i><span style='mso-fareast-language:ZH-CN'><o:p> </o:p></span></i></p><p class=MsoNormal style='mso-margin-top-alt:auto;margin-bottom:12.0pt;text-align:justify'>Predavanje bo v slovenščini.<o:p></o:p></p><p class=MsoNormal style='mso-margin-top-alt:auto;margin-bottom:12.0pt'><strong><span style='font-family:"Calibri","sans-serif";color:red'>Lepo vabljeni!</span></strong><strong><span style='font-weight:normal'><o:p></o:p></span></strong></p><p class=MsoNormal><o:p> </o:p></p><p class=MsoNormal><o:p> </o:p></p></div></body></html>