Results: outer shell, inner shell, FLIERs A new 3D model The Photoionization Structure of NGC 2392 The Eskimo Planetary Nebula Jonathan Sick (former Rice undergrad ...
Upflow in the Plage Region Associated with an X-class Flare. Shinsuke Imada (NAOJ) ... Observe the effect of the X class flare in Plage region with EIS ...
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 ...
Herschel telescope-coronagraph. with 175, 304 A bands having off-axis ... Observations of solar EUV-corona by the Herschel telescope in the coronagraphic mode ...
Daniel Stern (JPL) Lya. Lya. Lya. Lya. z=4.5. z=4.5. z=4.5. z=4.5. Keck/DEIMOS (Dawson et al. 2004b) ... 20% - 35% of the Lya-emitters in the spectroscopic ...
in a few arcsecs fov, there are significant changes: ... hot plasma ejecta or propagation of heating process to taller loops. log T = 6.8. log T = 7.2 ...
On the slow rise of quiescent prominences prior to their eruption ... cadence: 1 frames every 6 hours. CME watch: 4-5 frames per hour. High cadence images: ...
... et al. (2004) SOHO prominences. Photoionisation cross ... SOHO/EIT image in 304 A (left) and 195 A (right) overlaid as contours over an Yohkoh/SXT image. ...
New detailed star formation histories of all classic Local Group dwarfs ... Primordial gas does not cool efficiently in halos with T 104 K but we may also ...
Martins et al. in press. 6. Bouret et al. 2003. 2. Hillier ... Martins et al. 2005. Steep turn in MWM at log(L/L?) 5.25. SMC O stars. GAL, LMC, SMC O stars ...
to model the observations. Found since to work across all galaxies Ciardullo (03) ... for PNLF bright end in elliptical ( 10Gyr) galaxies? Possible explanations...
Database of potentially nearby PNe Improved integrated fluxes in Ha and [OIII] ... H. Bond / HST/ NASA AAO/UKST Survey Credit: ESA/ESO/NASA AAO/UKST Survey ?
Spectra 77 QSOs z=2 from Lick Kast spectrograph. Measured mean absorption from Ly-alpha in IGM. ... Lick 250 km/s. 24 QSOs HIRES 8 km/s. Removed mean metal ...
Requirements of technical systems V.Parma, TE-MSC Outline: Introduction Systems involved Cryogenic system Super-conducting bus bars Beam vacuum Other requirements
ATLAS CCD DE EST NDARES OB DE CLASIFICACI N ESPECTRAL. OBSERVADAS CON REOSC ... Est ndares de TE observadas en el azul-rojo con el fin de ampliar los criterios ...
2. Using the Ha surface brightness radius relation to generate a volume-limited ... Needed a statistical distance technique that was applicable to any PN. ...
1. Preliminary Airworthiness. Design Review for FIFI LS ... Engineers: H. Dohnalek (Design engineer, cryo/mechanics) G. Kettenring (Support engineer, FE modeling) ...
Jet-Gas Interactions in Seyfert Galaxies Mark Whittle (Virginia) David Rosario (Virginia) John Silverman (Virginia) Charlie Nelson (Drake) Andrew Wilson (Maryland)
Collimated ejections from binary central stars. Water maser emission in ... Precession period ~ 475 yr (D ~ 1.9 kpc, Palen et al. 2002) HST. Hu2-1 and IC4846 ...
The Off-Plane Option for the Reflection Grating Spectrometer Webster Cash University of Colorado Radial Groove Gratings An Off-plane X-ray Spectrum Off-plane ...
Must raster with slits for high spectral resolution. Can image with slots ... spectral imaging or optimized raster scanning for high spectral resolution ...
Unkown stellar mass loss at low metallicity. Henny Lamers ... Martins et al. 2004. Black = Gal. Red = LMC. Blue = SMC. ?L relation breaks down at log L 5.3 ! ...
Accurate: Comprehensive set of rays. Coronal physics. Equation of state ... v(k) = (k P(k))1/2. Velocity driving for corona sims. Voronoi tessellation. ensemble ...
REW 0.3 Angstrom ... REW=1 Angstrom black absorption 107 ... Only have analyzed 243 MgII systems with kinematically extreme absorption (REW 2 Angstroms) ...
Old population ( 2 Gyr): 4000 Ang break and other Lick indices. SSP: spectral evolution ... 5. Lick Indices : age/metallicity. CSF vs IB: RSG features. Mayya ...
Bona-fide BALQSOs appear have intrinsically blue optical ... Bona-fide BAL troughs are found in quasars with certain SEDs (blue, large blueshift, X-ray weak) ...
All galaxies have nuclear black holes. Those currently ... Gj ~ am Gem ~ 2-5 Gem. am = covering factor loss ; drag loss. Fj = Gj/Tage ~ 2-5 x 1033 dyne ...
Xi'an, October 2006. Note: the text accompanying this talk can be found at astro-ph ... nucleation of organic ice mixtures by UV photolysis (Kouchi et al. 2005) ...
B 5 ions at ~ separatrix sampled and Ti ~ 80 eV (so it appears they are ... don't know the limits of its use (how far inside the separatrix, density range...
NOTES: The Lives of Stars Gestation, Birth, and Youth: 1. The womb: Stars are born in dense molecular clouds.--The interstellar medium must be dense enough so H atoms
The Birth and Assembly of Galaxies: the Relationship Between Science ... J.-D. Smith, Casey Papovich, Romeel Dav , Jean Brodie, Bev Oke, Brad Whitmore, Rob Kennicutt ...
David Tytler, David Kirkman, Nao Suzuki, Dan Lubin, Xiao-Ming Fan, Scott Burles, ... Depends on fraction of gas in stars, IMF, infall of gas with primordial D/H ...
What can we learn about... The obscured sources responsible for the peak ... z~1 with D.Alexander, R.R. Chary ... Unified scenario: Compton Thick AGNs = edge-on ...
Narrow-band imaging ... But Keck long-slit & narrow-band surveys in 1998 (Cowie & Hu, Hu et ... Since then, narrow-band surveys using mostly 4-m class ...