Superbubbles PowerPoint PPT Presentations
All Time
Recommended
Probing the Galaxy with Superbubbles 3D Simulations
| PowerPoint PPT presentation | free to view
The Orion Nebula is one of the most prominent. ... Were it not for the radiation of the O stars, the Orion Nebula would be invisible. ...
| PowerPoint PPT presentation | free to download
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 ...
| PowerPoint PPT presentation | free to download
Observations of ISM Bubbles
| PowerPoint PPT presentation | free to view
Elisabete M. de Gouveia Dal Pino (IAG-USP) Introduction ... Detailed model to determine HE (Melioli & de Gouveia Dal Pino, A&A, 2004) HE. SN. Shock wave ...
| PowerPoint PPT presentation | free to download
Specification of the time or radius determines the rest of the structure. ... Multiple SNR expands like wind-driven bubble with Lmech=NSNESN/?tSN ...
| PowerPoint PPT presentation | free to download
Or cold gas in the vicinity of galaxies and cosmic. filaments (Pfenniger & Combes 94) ... Mass profiles for dwarf Irr galaxies dominated by DM ...
| PowerPoint PPT presentation | free to download
Constraints on the GCR Source Derived from Isotopic Abundance Measurements Washington U. Bob Binns Jay Cummings Louis Geer Georgia deNolfo Paul Hink
| PowerPoint PPT presentation | free to download
For hydrogenic ionic stages, the ionization cross-section (Dopita ... Magellanic Stream gas (Weiner & Williams 1996) Optical depth to ionizing radiation t = 3 ...
| PowerPoint PPT presentation | free to download
Mar 10: Oral presentation of final project proposals to class. ... ixx - include the following at line xx ... For next class read for discussion: Ferri re, 2002, ...
| PowerPoint PPT presentation | free to download
A lot of processes inject small scale fields in the ISM. stellar dynamos combined ... large scale flows amplifying a primordial field. inverse turbulent cascade ...
| PowerPoint PPT presentation | free to download
The ISM holds the key to understanding star formation ... Is there mass and energy exchange between the disk and extragalactic space? Observing Goals: ...
| PowerPoint PPT presentation | free to download
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. ...
| PowerPoint PPT presentation | free to view
The Sun and other stars are commonly characterized by the radiation they emit. ... But the realization that stars could also have a continuous wind dates from the ...
| PowerPoint PPT presentation | free to download
The Hot ISM K.D.Kuntz The Henry Rowland Dept. of Physics The Johns Hopkins University and NASA/LHEA
| PowerPoint PPT presentation | free to download
The heating rate due to photo-electron ejection from grains is significant in ... Swap the x and y axes. log n. log T. 2. 3. 4. 5. log n0. L G. L G. G L ...
| PowerPoint PPT presentation | free to view
Several arrays of ground-based detectors achieve a sensitivity 1/100 of the flux ... view ~ 1 steradian) MILAGRO (LosAlamos, USA), Tibet ARGO (Yang Ba Jing, Tibet) ...
| PowerPoint PPT presentation | free to view
But the realization that stars could also have a continuous wind dates from the ... But for some stars -- e.g. during the Red Giant phase of a solar-mass star, or ...
| PowerPoint PPT presentation | free to download
... search has been MERLIN 'Key Project' Extrinsic ... WSRT and VLA support MERLIN results ... No clear detections of microlensing effects seen in MERLIN data ...
| PowerPoint PPT presentation | free to download
Bear Stearns, Citigroup, Merrill, UBS, Et. Al. Housing/Mortgage Superbubble ($2-$3 Trillion) ... Stock Prices Fall Faster Than EPS Estimates Decline ...
| PowerPoint PPT presentation | free to view
Approaching NGC 3079 with VLBI (Are Seyfert Jets Green?) Enno ... HST Chandra, Cecil et al. in prep. / NASA. B-VLA 1.4 GHz, Duric et al. 1983. 2 kpc ...
| PowerPoint PPT presentation | free to download
Local Bubble & Beyond: Philadelphia. 1 ... Local Bubble & Beyond: Philadelphia. 5. X-ray Shadowing. RASS keV map near our pointings ...
| PowerPoint PPT presentation | free to view
soft merging ( la Sagittarius dwarf) ... dynamical equilibrium: a suitable scenario to ... role of DM halos: self-regulated evolution; exponential profiles ...
| PowerPoint PPT presentation | free to download
... in stellar clusters / OB associations. True ages ... proper motion aligned within 5 degrees ... Possible origin in one of the Cygnus Superbubble OB associations ...
| PowerPoint PPT presentation | free to view
Boundary Conditions of the Heliosphere. Priscilla Frisch, University of Chicago ... Void affects heliosphere boundary conditions. 5. RADIATIVE TRANSFER MODELS ...
| PowerPoint PPT presentation | free to view
HI in Dwarf Galaxies ... HI dispersions: why the same in dwarfs and spirals? ... the HI disk is thicker ...
| PowerPoint PPT presentation | free to view
NASA, ESA, N. Smith (University of California, Berkeley) and the Hubble Heritage ... quasar absorption lines. intergalactic radiation field; escape of ionizing photons ...
| PowerPoint PPT presentation | free to view
GASKAP. the Galactic ASKAP Spectral line survey. Coordinators - Steering Committee ... Snezana Stanimirovic (U Wisc), Jacco van Loon (U Keele) ...
| PowerPoint PPT presentation | free to view
