'Continuum emission' presentation slideshows

795 views • 58 slides

Bielby & Shanks 2007 MNRAS submitted

Bielby & Shanks 2007 MNRAS submitted. Chanda sample of 38 z=0.3 clusters. ROSAT sample of 30 low z clusters. Interstellar Neutral Hydrogen Emission Structure and Radio Frequency Continuum Radiation (WMAP) Signals. Gerrit L. Verschuur Physics Department University of Memphis.

382 views • 30 slides

Using the ? -ray Background as a Path to Mapping Dark Matter Clustering in the Universe

Using the ? -ray Background as a Path to Mapping Dark Matter Clustering in the Universe . Eiichiro Komatsu University of Texas at Austin PPC07@Texas A&M, May 18, 2007. K. Ahn & EK, PRD, 71, 021303R (2005); 72, 061301R (2005) S. Ando & EK, PRD, 73, 023521 (2006)

356 views • 26 slides

Cosmic ? -ray Background from Dark Matter Annihilation in the Large-scale Structure

Cosmic ? -ray Background from Dark Matter Annihilation in the Large-scale Structure. Eiichiro Komatsu University of Texas at Austin Cosmology Seminar@MPA August 21, 2007. K. Ahn & EK, PRD, 71, 021303R (2005); 72, 061301R (2005) S. Ando & EK, PRD, 73, 023521 (2006)

398 views • 26 slides

Hiroshi Imai (Joint Institute for VLBI in Europe) Anuj P. Sarma (Eastern Kentucky University)

European Workshop on Astronomical Molecules Zwolle, the Netherlands in 19 February 2004 The Kinematics, Physical Condition and Magnetic Field of the W3 IRS5 Region. Hiroshi Imai (Joint Institute for VLBI in Europe) Anuj P. Sarma (Eastern Kentucky University).

370 views • 23 slides

Astronomical Spectroscopy

Astronomical Spectroscopy. Astronomical Spectroscopy. Astronomical spectroscopy is done by attaching a spectrometer to a telescope A spectrometer is a device separates the individual wavelengths of the incoming light and measures the intensity of each

914 views • 23 slides

Indirect Dark Matter Search at Intermediate Mass Black Hole with the MAGIC Telescope

Indirect Dark Matter Search at Intermediate Mass Black Hole with the MAGIC Telescope. M. Doro 1(*) , H.Bartko 2 , G.Bertone 3 , A.Biland 4 , M.Gaug 5 , M.Mariotti 1 , F.Prada 6 , M.Rissi 4 , M.Sanchez-Conde 6 , L.S.Stark 4 , F.Zandanel 1 on behalf of the MAGIC Collaboration #

131 views • 1 slides

Imaging Arp 220 in CO 6-5 and dust at 100 pc resolution with ALMA

West Nucleus. East Nucleus. SiO absorption. 5085 km/s. 5135 km/s. 5185 km/s. 5235 km/s. 5285 km/s. 5335 km/s. 5385 km/s. 5435 km/s. 5485 km/s. 5535 km/s. 5585 km/s. 5635 km/s. Imaging Arp 220 in CO 6-5 and dust at 100 pc resolution with ALMA

135 views • 1 slides

Very Small Dust Particles and Chemistry in Photodissociation Regions: from ISO to Spitzer

134 views • 1 slides