'Early type' presentation slideshows

Raffaella Morganti (Astron, NL) C. Tadhunter ,T. Oosterloo, B. Emonts, J. Holt and many others

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MALARIA

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Galaxies in clusters and their progenitors

Galaxies in clusters and their progenitors. Pieter van Dokkum (Yale). General properties of cluster galaxies. Morphology-density relation In core approx. 80% are E and S0 galaxies. (Dressler 1980). General properties of cluster galaxies. Cluster galaxies follow tight scaling relations:

646 views • 48 slides

Fitting: The Hough transform

739 views • 46 slides

SFR and COSMOS

SFR and COSMOS. Bahram Mobasher + the COSMOS Team. COSMOS offers:. Extensive multi-waveband surveys from radio to X-ray Large area coverage ( 2 sq. deg.) HST/ACS morphologies (B/D, Sersic, concentration, asymmetry, clumpiness)

785 views • 43 slides

452 views • 39 slides

386 views • 30 slides

Multiwavelength Properties of the SDSS Galaxies in Various Classes

Feb 19, 2008 Joon Hyeop Lee 1 , Myung Gyoon Lee 1 , Changbom Park 2 , Yun-Young Choi 2 1 Seoul National University 2 Korea Institute for Advanced Study. SDSS-KSG Workshop. Multiwavelength Properties of the SDSS Galaxies in Various Classes. Introduction.

365 views • 23 slides

Multi-wavelength Properties and Environments of the SDSS Galaxies divided into Fine Classes

September 16, 2009 Joon Hyeop Lee Korea Astronomy and Space Science Institute Co-workers: Myung Gyoon Lee (SNU), Changbom Park (KIAS), Yun-Young Choi (ARCSEC ). KASI Colloquium. Multi-wavelength Properties and Environments of the SDSS Galaxies divided into Fine Classes.

304 views • 22 slides

The galaxy luminosity function & its evolution probed with Chandra

The galaxy luminosity function & its evolution probed with Chandra. Ioannis Georgantopoulos (NOA) Panayiotis Tzanavaris (NOA) Antonis Georgakakis (ICL). XLF importance : why probing X-rays ?. Unique probe of X-ray binaries and hot gas in normal galaxies:

345 views • 22 slides

DENVER FIRE ALARM TEST

DENVER FIRE ALARM TEST. FIRE ALARM SYSTEMS AND FUNDAMENTALS. Numbering System Does not use the NEC format Uses the standard NFPA format for numbering Advantages and Disadvantages Key Chapters for the Test Chapter 3 Definitions Chapter 10 Fundamentals Chapter 12 Circuits and Pathways

456 views • 19 slides

Color Magnitude Relations of early type galaxies in galaxy clusters

SDSS KSG Workshop 2007. Color Magnitude Relations of early type galaxies in galaxy clusters. 20 Feb 2007 Taehyun Kim , Narae Hwang, & Myung Gyoon Lee. Department of Physics and Astronomy, Seoul National University. Abell 168, z=0.045. Out of the blue line, they are not member galaxies.

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SEMINAR REPORT ON ROTARY ENGINE

SEMINAR REPORT ON ROTARY ENGINE. SUBMITED BY: SATYA NARAYAN BEHERA MECHANICAL ENGG. 8 TH SEMISTER. CONTENTS. INTRODUCTION WORKING PRINCIPLE MATERIAL FUEL CONSUMPTION & EMISSION ADVANTAGES DISADVANTAGES APPLICATION CONCLUSION. INTRODUCTION.

2.71k views • 18 slides

Infrared Luminosity Function of the Coma Cluster

Infrared Luminosity Function of the Coma Cluster. Lei Bai George Rieke Marcia Rieke Steward Observatory. Background. Infrared emission from galaxies: late-type galaxies ==> strong early-type galaxies ==> weak

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The Dirt on Dry Mergers

277 views • 17 slides

Angela Bongiorno Max Planck Institut fuer E xtraterrestrische Physik (MPE)

Optically Selected Type-2 AGN from the 10k zCOSMOS sample. Angela Bongiorno Max Planck Institut fuer E xtraterrestrische Physik (MPE). AGN8 Torino 19-22 May. Collaborators: Marco Mignoli (INAF-Osservatorio Astronomico di Bologna)

327 views • 16 slides

RAM (Random Access Memory)

532 views • 11 slides

Node organization Network activities and scientific highlights so far

MAGPOP The Italian node (INAF+SISSA). Node organization Network activities and scientific highlights so far. INVOLVED INSTITUTES. Node is scattered both from a geographic ( Padova + Trieste : 180 km) awa from an institutional point of view ( INAF + SISSA )

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Properties of Barred Galaxies in SDSS DR7 - OPEN KIAS SUMMER INSTITUTE -

89 views • 1 slides