'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:

423 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

403 views • 27 slides

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

360 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

360 views • 20 slides

Observing Molecules in the EoR

307 views • 19 slides

Constraints on progenitors of Classical Novae in M31

363 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

367 views • 13 slides