'Dust emission' presentation slideshows

Preparation to the CMB Planck analysis: contamination due to the polarized galactic emission

635 views • 49 slides

What we look for when we look for the dark gas *

What we look for when we look for the dark gas *. John Dickey Wentworth Falls 26 Nov 2013. *Wordplay on a title by Raymond Carver, "What we talk about, when we talk about love". Summary:

562 views • 48 slides

Supernova 1987A at 25 years

Supernova 1987A at 25 years. TOPICS. Highlights of the past 25 years Outstanding mysteries and surprises What we can expect to learn, sooner and later. Supernova Energy Sources.

557 views • 48 slides

Why, How, and How we Figure Out Where New Stars Form

536 views • 48 slides

Protostellar/planetary disk observations (and what they might imply)

468 views • 38 slides

Removing foregrounds from CMB maps using non- Gaussianity measurement

Removing foregrounds from CMB maps using non- Gaussianity measurement. Dr. Rajib Saha Assistant Professor Physics Department IISER Bhopal. A FOREGROUND CLEANED CMB MAP FROM NON-GAUSSIANITY MEASUREMENT Rajib Saha Accepted in ApJL , (arxiv:1105.6298) .

385 views • 30 slides

ASKAP Continuum S urveys of Local Galaxies

392 views • 30 slides

Basic Concepts

Basic Concepts. An interferometer measures coherence in the electric field between pairs of points (baselines). Direction to source. wavefront. c t. Bsin ?. ?. B. T2. T1. Correlator.

324 views • 23 slides

WAM Foam: asphalt pavements at lower temperatures

WAM Foam: asphalt pavements at lower temperatures. WMA TWG, 12 December 2007, Hunt Valley - MD. WAM Foam. Basic Concept & History Field Experience Emission Reduction US Perspective. Basic Concept . Hard asphalt component. PG 64-22. Soft asphalt component. Viscosity. Pa.s. 100000.

485 views • 22 slides

Using the CMAQ Model to Simulate a Dust Storm in the Southwestern United States

The 6 th CMAS Workshop. Using the CMAQ Model to Simulate a Dust Storm in the Southwestern United States. Daniel Tong $ , George Bowker * , Rohit Mathur + , Tom Pierce + , Shaocai Yu $ , Dale Gillette +.

374 views • 21 slides

Constraints on a Universal IMF 1 from the Entire Stellar Population 2,3

Constraints on a Universal IMF 1 from the Entire Stellar Population 2,3. Ivan Baldry. Johns Hopkins University working with Karl Glazebrook. 1 Assuming a universal IMF and constraining the upper-mass IMF slope (M >~ 1 solar mass).

287 views • 20 slides

Press conference

348 views • 18 slides

250 views • 17 slides

The Crab Nebula in the Infrared: A Review

The Crab Nebula in the Infrared: A Review. PAOLO PERSI. 1. OUTLINE. Why Infrared Observations of the Crab A brief history of the IR observations of the Crab Infrared polarimetric imaging of the Crab Future IR observations of the Crab. 2. Why IR observations of the Crab. Chandra X-ray

354 views • 16 slides

IR Shell Surrounding the Pulsar Wind Nebula G54.1+0.3

IR Shell Surrounding the Pulsar Wind Nebula G54.1+0.3. SNRs and PWNe in the Chandra Era Boston, July 8, 2009. Tea Temim (CfA, Univ. of MN) Collaborators: P. Slane, S. Reynolds, J. Raymond, K. Borkowski. Outline.

263 views • 15 slides

Supernova Dust and Ejecta Illuminated by Pulsar Wind Nebulae

Supernova Dust and Ejecta Illuminated by Pulsar Wind Nebulae. European Space Astronomy Centre (ESAC) May 23, 2013. Tea Temim (GSFC/ORAU). Evolution of PWNe inside SNRs. Ejecta/Dust Emission :

322 views • 14 slides

photo: Keith Vanderlinde

Detection of tensor B-mode polarization : Why would we need any more data?. photo: Keith Vanderlinde. If the measured r angular-spectrum leads to any surprising physics, it is crucial to establish beyond any doubt that the signal originates in the CMB.

204 views • 13 slides

ALMA Science Workshop May 14-15, 2004 Star and Planet Formation Breakout Session

ALMA Science Workshop May 14-15, 2004 Star and Planet Formation Breakout Session. Facilitators: Doug Johnstone & Debra Shepherd. Science & the DSRP. Detailed summary of representative proposals: Claire Chandler , DRSP 2.1.6, OTF survey of large field

211 views • 8 slides

CPP-II Wagon Tippler without DS System

CPP-II Wagon Tippler without DS System . Emission of Dust at Start of Tippling. Dust during unloading. NOHS Official measuring DUST emission at Wagon Tippler. NOHS Official in discussion with Wagon Tippler staff.

367 views • 5 slides

Where is the Silicate Emission Region in AGNs?

I. Silicate Dust Features in AGNs

88 views • 1 slides