Magellanic PowerPoint PPT Presentations

Magellanic Clouds

Radiocontinuum PNe in the Magellanic Clouds

Contours: MAGMA CO data. Greyscale: IR excess map. Tracing H2 with NIR Extinction. Method outline: ... Peak HI Temp (contour) on Integrated CO. CO vs. HI in LMC ...

2 Gaussians fit better than 5 point sources despite smaller number of parameters ... (consistent with difference between galactic and LMC SN rate) Average ...

The MS in History (very abridged) Henrietta Leavitt and the SMC Cepheids ... And dust: 1% of ISM mass 0.1mm. heating/cooling. catalyst for molecule formation ...

Classical novae in the Magellanic Clouds. Elena Mason, ESO science day ... He/N 2500 km/s flat topped/jagged days, neon [Ne V,III] coronal [FeX,VII] no lines ...

Outline Background- RR Lyrae Variables The Hertzsprung-Russell diagram Globular Clusters Satellite Galaxies Galaxy Formation ... Globular Cluster H-R ...

The Spitzer View of the Small Magellanic Cloud

Understand the formation and spatial distribution of elements in star forming ... No lines of Ne and Ar in the solar photosphere ...

An important breeding colony is Isla Martillo in the Beagle Channel, Argentina ... All 22 penguins left Beagle Channel in an easterly direction ...

Using filters on a catalog to visualize the shell characteristics ... Choose the Vizier Catalogs folder on the right. Type ' shells ' in the free text zone ...

X-ray contours on an Ha image ... Radio image and X-Ray contours of the SNR N157B which is just becoming a composite remnant. ...

... Spirals in Ursa Major and Canes Venatici: Global Properties. Kwayera Davis (College of Charleston) Advisor: Eric Wilcots (University of Wisconsin-Madison) ...

The Orbital Evolution of the Magellanic Clouds and the Implications for the ... Brant Robertson. T.J. Cox. Roeland P. van der Marel. Charles Alcock ...

Title: Cyberinfrastructure to Support Science and Data Management for the Dark Energy Survey Author: Choong Ngeow and Joe Mohr Last modified by

LAB survey. Bruns et al. 05. Braun & Thilker 04 ... Latest observational (HI) results: ... If in free expansion, mean expansion time 10 Myr, very short. ...

Covers Chapters 6 (Telescopes), 14 (The Sun), 15 (Surveying Stars) ... Supernova 1987A blast wave. Large Magellanic Cloud. Small Magellanic Cloud. Spectral Lines ...

The Crab Nebula. The Milky Way. The Large Magellanic Cloud. The Small Magellanic Cloud ... Our solar system lies on the outer part of one of its spiral arms. ...

Introduction. The Magellanic System, comprising the Small and Large Magellanic ... In contrast to other phases of the ISM, the molecular gas in the Magellanic ...

Nubecula Major IN GLORIOUS Adric Riedel Outline Basic Facts Discovery Morphology Its place in the Local Group Relation to the Small Magellanic Clouds As compared to ...

... immediately Tiger Magellanic Penguin Javan Rhinoceros Giant Panda Blue-fin Tuna Monarch butterfly Leatherback Turtle Mountain Gorilla Polar Bear Pacific ...

For hydrogenic ionic stages, the ionization cross-section (Dopita ... Magellanic Stream gas (Weiner & Williams 1996) Optical depth to ionizing radiation t = 3 ...

Tasmanian forest. New Zealand tree ferns. New Zealand Kauri tree. Animals ... Tasmanian devil. Kakariki. Magellanic woodpecker. People ...

O-16, Ne-20, Mg-24, Si-28, S-32, Ar-36, Ca-40, Ti-44, Cr-48, ... N49 in the Large Magellanic Cloud. Cassiopeia A. Supernova. 1987A. In the Large Magellanic Cloud ...

Orion Orionis. Seeing the Constellations. Seeing the Constellations. Seeing the Constellations ... South of Orion. The Magellanic Clouds. An Ex-Constellation ...

The GALFA-HI Survey will map the entire Arecibo sky (shown between the red lines ... Magellanic Stream: The HI velocity field of the Magellanic System from the ...

Do bipolar PNe really have more massive progenitors? Central stars? Eva Villaver (STScI/ESA) X. Outline. Central star masses. MageLlanic Clouds. RESULTS in the Galaxy ...

N81 in Small Magellanic Cloud. Double Bubble N30B. Gomez's Hamburger ... Orion Nebula's Trapezium Cluster. Southern Crab Nebula (He2-104) Galaxy Cluster Abell 1689 ...

unless there is a mysterious repulsive force to balance the gravitational attraction ... closest neighbors in the Local Groups: Andromeda, Magellanic Clouds etc. ...

COBE near-infrared image of the Milky Way. NGC 891. Magellanic clouds. Fornax dwarf galaxy. Leo I dwarf galaxy. M31 = Andromeda galaxy NGC 205 M32 ...

Below, Tarantula nebula, 30 Doradus. in the Large Magellanic Cloud. Right: ? Carinae nebula, in ... 8. 30 Doradus, the Tarantula. nebula, a giant. HII nebula ...

Large and Small Magellanic Clouds (LMC and SMC) are ... Generally gas poor with old red stars. Spirals come in two types: normal (S) and barred (Sb) ...

Supernova 1987A in the Large Magellanic Cloud 1994 1998 Expanding debris from star. Speed almost 3000 km/sec! Light from supernova hitting ring of gas, ...

Large Magellanic Cloud (satellite to Milky Way) . Distance=50 kpc. Pic:http://antwrp.gsfc.nasa.gov/apod/ap010804.html ... These are the closest galaxies ...

some penguins will spend several years at sea before returning to land ... Magellanic, Humboldt, Galapagos, & Blackfoot Penguins are the only species that ...

Stellar formation in Papillon Nebula in Large Magellanic Cloud. Lagoon Nebula ... Birthplace of massive stars: 30 Doradus Nebula. Magnified view of 30 Doradus Nebula ...

Indian Institute of Astrophysics, Bangalore, INDIA (Evidence of a counterrotating core in the LMC: ... The Large Magellanic Cloud (LMC) has been studied ...

... Galaxy, extragalactic stellar populations and history (Magellanic Clouds) from ... 450 m opens 50% of time deep extragalactic surveys (synergy with ALMA) ...

Jacco van Loon. Keele University. Dust wind structure. Radiative equilibrium ... van Loon et al. (1999) new MSX sample. Superwind mass-loss rates ...

Paucity of young HMXBs. Popov et al. (1998) (Z=0.02, log(Lmin)=33) ... Paucity of young HMXBs. Evolution of HMXBs population: observational constraints ...

Our New View of the Local Group

Paul Jones (UNSW) Molecular Lines from dense molecular clouds regions (and OH 1720) ... with red giant stars, and hundreds of masers in star formation regions. ...

Final results on galactic dark matter from the EROS2 microlensing survey

For recent O VI survey, see Fox et al (2004 ApJ 602, 738) ... Grey contours: NHI integrated between -450 to 400 km/s (excluding local HI) ...

how to determine the physical laws that govern the propagation of ... The parabola results from a square law relationship between delay and Doppler shift. ...

10-day exposure on an apparently empty field in the sky. Even seemingly empty regions of the sky contain thousands of very ... The Extragalactic Distance Scale ...

STREGA & STEP are surveys in the context of INAF-OACN GTO. Small and focused surveys ... STRructure and Evolution of the GAlaxy. P.I.: Marcella Marconi ...

Dwarf galaxies

RAG Journal Club 11 Oct 2006. Observation of structure on a wide range of scales ... Earth Orbit Synthesis of Intra-Day Variables: Dennett-Thorpe and de Bruyn ...

heating-cooling balance and the phases of the ISM ... Brogan et al. 2006 Ap. J. 130, 698. 3C138 Continuum. 21-cm absorption. Optical Absorption Lines ...

While I was in the service of the Spanish King and Queen, I ... Moonwalk! BETTER THAN BATMAN! GOOD MORNING! CENSORED (UNDER) 18S. BE. WARNED, THE. CHICKENS ...

GASKAP. the Galactic ASKAP Spectral line survey. Coordinators - Steering Committee ... Snezana Stanimirovic (U Wisc), Jacco van Loon (U Keele) ...

Gravitational Microlensing The SuperMACHO survey My work Image-Processing ... This can happen even in the case where the source is not obscured by the lens What is ...

The big problem in cosmology is ... Radioactive dating of stars showed that no stars were formed earlier than 200, ... The Missing Mass and Dark Matter ...

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