its key objectives an accurate, physically motivated explanation ... organic aroma. Most types of carbonaceous. chondrites (and there are lots of types) ...
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Steve Kent. Rita Kim. Tim Mcay. Erin Sheldon. Bob Nichol. Chris Miller. Tomo Goto. Neta Bahcall ... Steve Kent. Scott Dodelson. Josh Friemann. Tim Mckay. Erin ...
Fe mass in the central peak normalised to K band luminosity of central galaxy ... Galaxy groups, like cool core clusters, have central abundance peaks dominated ...
Then helium (He) was also formed in the Big Bang, when the Universe was 3 20 minutes old. The temperature was then just right ... Tolstoy's view in 1889 ' ...
Volatile Abundances in Basaltic Magmas & Their Degassing Paths Tracked by Melt Inclusions ... is a necessity and represents a main challenge for the next few years. ...
... neutron capture relative to the -decay timescale. Mass transfer from low ... Rapid neutron capture relative to the -decay timescale. Neutrino wind from SNe II ...
Steve Majewski (UVa), Katia Cunha, Verne Smith (NOAO), David Mart nez-Delgado (IAC) ... Sgr core of today differs from Sgr core of 'yester- gigayears' ...
Mei-Yin Chou (UVa - Ph.D. thesis), Katia Cunha, ... Testing the connection to the Monoceros stream. ... Tri-And Star Cloud not chemically linked to Monoceros. ...
5 out of 7 stars have essentially solar CNO abundances (weak 3rd dredge-up because of low mass? ... LS V 4621 (=Sh2-216): CNO and He 1-2 dex subsolar ...
Cluster abundances averaged from XMM-Newton observations, fit with a combination ... Surprisingly, no combination of these two sources explains the observed ratios ...
Pilyugin et. al (2003, A&A, 401, 557) find O/H = 8.52 dex in the solar vicinity ... was formed, there has been an 0.13 dex increase in oxygen abundance of the ISM ...
AGB star intershell abundances inferred from analyses of extremely hot H-deficient post-AGB stars Klaus Werner Institut f r Astronomie und Astrophysik Universit t ...
JENNIFER SOBECK, FRANCESCA PRIMAS, CHRIS SNEDEN. EUROPEAN ... Presence of hyperfine ... with the Ultraviolet and Visual Echelle Spectrograph (UVES) ...
Blue Channel spectroscopy of. quasar absorption lines: Metal abundances and dust in DLYAs ... Chandra X-ray Spectroscopy of absorption: Soft X-ray absorption ...
... only from higher-excitation Si I yellow-red lines ... n-capture, recent lab transitions. Three groups contribute especially: Lund, Liege, Wisconsin ...
We discuss periodical cicada (Magicicada) Brood VII, which is becoming extinct ... Brood VII periodical cicada records. Filled circles: Magicicada present in 2001. ...
Overall good agreement with NOAO Fundamental Plane Survey ( ); (Smith et al. 2005) ... Center galaxies with 100 kim/s. Center with 50 100 km/s. Center with ...
Istituto Nazionale di AstroFisica (Istituto di Astrofisica Spaziale e Fisica Cosmica) ... though the ground and the metastable 26Al states are properly taken into ...
Mare basalt. 3.3 Ga. 14-15% MgO. near primary precursors to high TiO2 basalts. ... cumulate from a pre-mare basaltic melt. Exp method. spherule sample ...
MODIS was not designed to supply accurate middle-atmosphere ozone abundances. ... nadir to 65o and the seven zones based on the 11- m brightness temperatures ...
Two things occur simultaneously in space or time (both) ... Salmonid Watershed Assessment Model (SWAM) ... Predict relative salmonid abundances behind barriers ...
Solar model problem solved by the abundance of Ne in stars of local cosmos. Solar chemical abundances of O, C, N, Ne and Ar need to be reduced (Asplund et al. 2004) ...
Large Scale Survey & the Robert Stobie Spectrograph (RSS) on SALT ... Robert Stobie Spectrograph (RSS) Formerly the Prime Focus Imaging Spectrograph (PFIS) ...
Zr I, Ba II enhanced by 0.5 dex. Zr I, Ba II enhanced by 1.0 dex. Zr I & Ba II ... for s-process element abundance variations of at least 0.5 dex to be observed ...
Supervisors: Ana Inez Gomez de Castro. Isabella Pagano. COSPAR2008. Objectives. To detect the C, N, O lines in post-AGB (asymptotic giant branch) stars from UV spectra ...
LS coupling. No relativistic effects (no intercombination E1 transitions) ... stellar structure which Simulates HB or intermediate mass stars. Trend: Z Diff. ...
The first light nuclides were synthesized in a short time interval following the ... coincide, the abundance ratio He / H is either underestimated or overestimated ...
... N, Mg, Al, Ne, Fe & others (Munich Observatory N. ... tailored. modelling. Similar results for He, N, O Ne, Mg, Si, Fe. So far O, Mg & Si confirmed by ...
Loose collections of species that tolerate the same environmental conditions? ... of species should co-occur as one community transitions to another (ecotone) ...
Hard to discriminate between Ia models, but see extremes Hydra A / M87 ... Similar results in Hydra A. 4. Enrichment by winds. XMM-Newton RGS results ...
School of Physics, Peking University. Collaborators: Thomas Gehren (LMU) Keith Butler (LMU) ... The low mass unevolved stars have long lifetimes, some of them ...
Ni ABUNDANCE IN THE CORE OF THE PERSEUS CLUSTER: AN ANSWER TO THE ... Fabio Gastaldello (CNR-IASF, University of Milan-Bicocca) Silvano Molendi (CNR-IASF) ...
Impact of Fishing on the Abundance of Marine Species Rainer Froese IfM Kiel rfroese@ifm.uni-kiel.de Kathleen Kesner-Reyes MSI Quezon City kkesner_reyes@hotmail.com