'Gas fraction' presentation slideshows

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ALMA workshop ? ALMA ????????????????????????????? 2013 ? 2 ? 25 ? -26 ? ???????. ????????????????????????. ????? ???? ??????????? kkohno@ioa.s.u-tokyo.ac.jp. L(IR)=5x10 10 Lo SFR ~ 8 Mo/yr. Radio to IR spectrum of the starburst galaxy M82. Wavelength:. 10?m. 100?m. 1mm. 1cm. 10cm.

1.03k views • 77 slides

AGAR CORPORATION Process Measurement & Control

AGAR CORPORATION Process Measurement & Control. Multi-Phase Measurement Options Associated Problems. Basic Multi-Phase Flow Measurement Formulas. 1.2 - MPFM Formulas.

760 views • 47 slides

Supermassive black holes (SMBH) and formation of galaxies

507 views • 33 slides

Galaxy Formation: What are we missing?

Quenching ? : How to Move from the Blue Cloud ? Through the Green Valley ? and to the Red Sequence ? in 9 Easy Steps in the Face of Downsizing?. C. Steidel (Caltech). Galaxy Formation: What are we missing?. Some Questions:.

395 views • 31 slides

Desai et al. (2007)

Desai et al. (2007). Large variation in MIR spectra driven by PAH, H 2 O ice, hydrocarbon & silicate absorption 30-40% of the power of a typical ULIRG comes from an AGN. This rises with luminosity, dust temp, merger stage, etc.

472 views • 25 slides

CMB Constraints on the Intracluster Medium

CMB Constraints on the Intracluster Medium. Niayesh Afshordi Institute for Theory and Computation Harvard College Observatory. My Collaborators. Yen-Ting Lin University of Illinois Urbana-Champaign Princeton Alastair Sanderson University of Illinois Urbana-Champaign

331 views • 25 slides

The Building Up of the Black Hole - Stellar Mass Relation

The Building Up of the Black Hole - Stellar Mass Relation. Alessandra Lamastra. collaborators:. Nicola Menci 1 , Roberto Maiolino 1 , Fabrizio Fiore 1 , Andrea Merloni 2. 1 INAF - Osservatorio Astronomico di Roma. 2 Max-Planck-Institut fur Extraterrestriche Physik.

288 views • 20 slides

Missing Thermal Energy of the Universe

Missing Thermal Energy of the Universe. Niayesh Afshordi Institute for Theory and Computation Harvard College Observatory. My Collaborators. Yen-Ting Lin University of Illinois Urbana-Champaign Princeton Daisuke Nagai CalTech Alastair Sanderson University of Illinois Urbana-Champaign

317 views • 19 slides

347 views • 15 slides

What have we learned ? ( very briefly )

Sources of the CIB are found up to z~2 Not fully characterised beyond statiscial properties N(>S), n(z), SFR-M* Not understood theoriticalky (SAM, Hydro) CIB at higher redshift still unknown Hints from SMGs Study of CIBA: Very well measured H as not reached its potential

156 views • 3 slides