2 Gaussians fit better than 5 point sources despite smaller number of parameters ... (consistent with difference between galactic and LMC SN rate) Average ...
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 ...
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 ...
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 ...
... 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 ...
LAB survey. Bruns et al. 05. Braun & Thilker 04 ... Latest observational (HI) results: ... If in free expansion, mean expansion time 10 Myr, very short. ...
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. ...
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 ...
For hydrogenic ionic stages, the ionization cross-section (Dopita ... Magellanic Stream gas (Weiner & Williams 1996) Optical depth to ionizing radiation t = 3 ...
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 ...
Introduction. The Magellanic System, comprising the Small and Large Magellanic ... In contrast to other phases of the ISM, the molecular gas in the Magellanic ...
Orion Orionis. Seeing the Constellations. Seeing the Constellations. Seeing the Constellations ... South of Orion. The Magellanic Clouds. An Ex-Constellation ...
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 ...
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 ...
unless there is a mysterious repulsive force to balance the gravitational attraction ... closest neighbors in the Local Groups: Andromeda, Magellanic Clouds etc. ...
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, ...
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 Magellanic Cloud (satellite to Milky Way) . Distance=50 kpc. Pic:http://antwrp.gsfc.nasa.gov/apod/ap010804.html ... These are the closest galaxies ...
Large Magellanic Cloud has circulated our Galaxy for about 5 times at 50 kpc ... hole of mass m on a rosette orbit bound between pericenter r0 and apocenter 2r0. ...
some penguins will spend several years at sea before returning to land ... Magellanic, Humboldt, Galapagos, & Blackfoot Penguins are the only species that ...
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) ...
Paucity of young HMXBs. Popov et al. (1998) (Z=0.02, log(Lmin)=33) ... Paucity of young HMXBs. Evolution of HMXBs population: observational constraints ...
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. ...
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 ...
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 ...
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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