'Dense gas' presentation slideshows

ESAC report

ESAC report. Rebaselining Time Allocation procedure Other items ARC, EU-FP6: see T. Wilson. I. ALMA Rebaseling. Most of the ESAC and ASAC discussions over the last year focussed on the ALMA rebaselining; see ASAC reports October 2004, March 2005 and October 2005

570 views • 39 slides

Chapter 4: Light

477 views • 39 slides

Extragalactic Star Formation activity

496 views • 39 slides

Fingerprinting (ultra)luminous infrared galaxies

567 views • 37 slides

Extragalactic Star Formation into the ALMA Era (Beyond CO)*

Extragalactic Star Formation into the ALMA Era (Beyond CO)*. Yu GAO ? ? Purple Mountain Observatory, Nanjing Chinese Academy of Sciences. * Dedicated to the Memorial of Phil Solomon. Talk Outline. 1) Introduction: Massive Star Formation

433 views • 31 slides

CO luminosity for spirals, ULIRGs and high z EMGs ARAA6

Molecular Gas, Dense Molecular Gas and the Star Formation Rate in Galaxies (near and far) P. Solomon. Molecular Gas Mass as traced by CO emission and the star formation rate in spiral galaxies, LIRGS, ULIRGs and high z molecular galaxies (Early Molecular Galaxies, EMGs)

223 views • 22 slides

Turbulence, Feedback, and Slow Star Formation

Turbulence, Feedback, and Slow Star Formation. Mark Krumholz Princeton University / UC Santa Cruz Gas Accretion and Star Formation in Galaxies MPA/ESO/MPE/USM Conference 11 September 2007 Collaborators: Tom Gardiner, Jim Stone (Princeton) Todd Thompson (Princeton / Ohio State)

321 views • 21 slides

Connecting Dense Gas Tracers of Star Formation in our Galaxy to High-z Star Formation

Connecting Dense Gas Tracers of Star Formation in our Galaxy to High-z Star Formation. Jingwen Wu ( The Univ. of Texas at Austin ). Collaborators: Neal Evans (Advisor, UTexas at Austin) Yu Gao (PMO); Phil Solomon, Tom Mooney (SUNY-SB); Paul Vanden Bout, Yancy Shirley (NRAO).

271 views • 14 slides

A Systematic Survey of High-Mass Infall Candidates

206 views • 11 slides

IRAC/MIPS view of the ISM: PAHs dominate in IRAC

IRAC/MIPS view of the ISM: PAHs dominate in IRAC. Li & Draine (2001) dust emissivity model; only very strong (> 10 3 x avg.) radiation fields contribute to thermal emission at 8 ? m.

265 views • 9 slides

The Sun

235 views • 8 slides

ABSTRACT

Connecting Dense Gas Tracers of Star Formation in our Galaxy to High-z Star Formation Jingwen Wu & Neal J. Evans II (Univ. of Texas at Austin) ; Yu Gao (PMO); Phil Solomon, Tom Mooney (SUNY-SB); Paul Vanden Bout, Yancy Shirley (NRAO). ABSTRACT

132 views • 1 slides