'Molecular gas' presentation slideshows

575 views • 49 slides

Nearby Galaxies (mostly) at mm and IR wavelengths

Nearby Galaxies (mostly) at mm and IR wavelengths. Adam Leroy (MPIA Heidelberg) Christof Buchbender (IRAM Granada). Liberally plundering .ppt by: Eric Bell, Hans-Walter Rix, James Graham. Topics. A Broad Look at Nearby Galaxies Nearby Galaxies at Millimeter Wavelengths

545 views • 37 slides

Cooling flows and Galaxy formation

Cooling flows and Galaxy formation. James Binney Oxford University. Outline. Phenomenology of CFs Physics of heating Standard galaxy formation Galaxy formation revisted. collaborators. Len Cowie Gavin Tabor Henrik Omma Fathallah Alouani Bibi Carlo Nipoti Filippo Fraternali.

429 views • 31 slides

384 views • 29 slides

RGS spectroscopy of the Crab nebula

RGS spectroscopy of the Crab nebula. Jelle S. Kaastra Cor de Vries, Elisa Costantini, Jan-Willem den Herder SRON. Introduction. RGS Crab spectrum used for calibration purposes Here focus on astrophysics : ISM absorption. XMM-Newton OM (231, 291 , 344 nm) Courtesy A. Talavera, ESA.

373 views • 26 slides

Molecular gas dynamics in luminous infrared galaxies observed with the SMA

Molecular gas dynamics in luminous infrared galaxies observed with the SMA. Chris Wilson, McMaster University C. Wilson et al. 2008 (ApJS, in press), D. Iono et al. 2008 (submitted to ApJ). UGC5101. Mrk273. Molecular gas dynamics in luminous infrared galaxies.

444 views • 26 slides

Molecular Gas (Excitation) at High Redshift

Molecular Gas (Excitation) at High Redshift. Fabian Walter Max Planck Institute for Astronomy Heidelberg. A. Weiss ( MPIfR ) D. Downes (IRAM), D . Riechers (Caltech), C. Carilli (NRAO) , F. Bertoldi ( AIfA ) , P . Cox (IRAM), R. Wang (U Peking), E. Daddi (CES), Ran Wang (UA).

334 views • 25 slides

THE STAR FORMATION LAW I.

THE STAR FORMATION LAW I. THEORY AND APPLICATION TO NEARBY GALAXIES. Chris McKee. With:. Mark Krumholz, Adam Leroy,. Dekel60 Jerusalem December 15, 2011. Eve Ostriker, & Jason Tumlinson. Reionization. Heavy elements. Galaxy formation and evolution. Planet formation.

439 views • 24 slides

MX002: Molecular Gas in the LMC

MX002: Molecular Gas in the LMC. MX002 observers in 2005: Juergen Ott, Tony Wong, Erik Muller, Jorge Pineda, Min Wang, Annie Hughes. Talk Outline. the MX002 project observations in 2005 the molecular ridge near 30 Doradus: mass function, X-factor, line profiles, ASTE/Mopra

318 views • 23 slides

Masses of the Highest Redshift Quasars and Their Host Galaxies

Masses of the Highest Redshift Quasars and Their Host Galaxies. Hubble Fellowship Symposium 2008 STScI, Baltimore, MD March 10-12, 2008 Dominik A. Riechers California Institute of Technology. Hubble Fellowship HST-HF-01212.01-A. High Redshift Galaxy Zoo. z = 1000. Distant Galaxies:

413 views • 22 slides

A Far-Ultraviolet View of Starburst Galaxies Claus Leitherer (STScI)

361 views • 20 slides

Why are Some Brightest Cluster Galaxies Forming Stars?

303 views • 18 slides

An NH 3 Survey Program with the Radio Telescope of Hokkaido University

298 views • 16 slides

Lecture 4 - Interstellar Cloud Collapse

Lecture 4 - Interstellar Cloud Collapse . Topics to be covered: The Interstellar Medium Gravitational collapse Virial Theorem Jeans Instability. Interstellar Medium (ISM). Interstellar space is not empty - there is gas and dust in the galaxy.

684 views • 14 slides

HCO + in the Helix Nebula

HCO + in the Helix Nebula. Lindsay N. Zack Lucy M. Ziurys Department of Chemistry Department of Astronomy Steward Observatory Arizona Radio Observatory University of Arizona. Planetary Nebulae.

259 views • 14 slides

Molecular Gas at High Redshift

298 views • 14 slides

Henize 2-10

IC 10. NGC 253. Henize 2-10. COMPARISON OF GAS AND DUST COOLING RATES IN NEARBY GALAXIES E.Bayet : LRA-LERMA-ENS (Paris). Antennae. IC 342. M 83. NGC 6946. INTRODUCTION :. OBJECTS : warm and dense molecular clouds in the nuclei of 20 nearby galaxies with

276 views • 14 slides

The Fate of the X-Ray Emitting Gas in the Early-Type Galaxy NGC 5044

214 views • 12 slides

Molecular clouds in the center of M81

175 views • 9 slides

Molecular Gas and Dust in SMGs in COSMOS

Molecular Gas and Dust in SMGs in COSMOS. Left panel is the COSMOS field with overlays of single-dish mm surveys. Right panel is a 0.3 sq degree map at 1.3mm (Scott et al.) During Early Science, ALMA may be used to follow up all of these sources to identify the counterparts. .

136 views • 2 slides