'Sun yr' presentation slideshows

High energy neutrino astronomy: Challenges & Prospects

High energy neutrino astronomy: Challenges & Prospects. Eli Waxman Weizmann Institute, ISRAEL. High energy n ’ s: A new window. MeV n detectors: Solar & SN1987A n ’ s Stellar physics (Sun ’ s core, SNe core collapse) n physics >0.1 TeV n detectors:

415 views • 31 slides

Does Gas Cool From the Hot Phase? (onto galaxies)

Does Gas Cool From the Hot Phase? (onto galaxies). Hot Gas in/around Ellipticals: Lessons Learned Hot Gas Environment of the Milky Way and Local Group: Limits on Accretion Missing Baryons in Galaxies and Galaxy Groups. The MPA/ESO/MPE/USM 2007 Joint Astronomy Conference

394 views • 27 slides

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???????????? ???????????. ?? ?? ( ??????? ). ??. ???????????? DLA ???????????? ??????????????? ??? ( ???? ) ?????????? ???. 1. ????????????. ???? (H 2 ) ???????????? ?????????????. ??? ?????? H 2 ?? ???????????????? ????????????. H 2 ???????????. ????? (H 2 ). ????. ???.

342 views • 23 slides

Star Formation in High Redshift Submillimeter Galaxies and QSO Hosts

Star Formation in High Redshift Submillimeter Galaxies and QSO Hosts. Dieter Lutz MPE Elisabetta Valiante, Eckhard Sturm, Reinhard Genzel, Linda Tacconi, Mario Schweitzer, Andrew Baker, Hagai Netzer, Roberto Maiolino, Paola Andreani, Sylvain Veilleux

333 views • 20 slides

Observing Molecules in the EoR

297 views • 19 slides

Constraints on progenitors of Classical Novae in M31

342 views • 16 slides

Cas A ??????? ??????????

Cas A ??????? ??????????. ????? ???????????????????? ????? ?? ?? ( ?? ), ??? ( ????? ), ???? (IPMU), ? ???? ( ?? ), ???? (IPMU/ ?? ). 1-1. Introduction. ?? Dust in SNRs ? CCSNe are important sources of dust? ? formation of dust in the ejecta of SNe

346 views • 13 slides